TAP_SCHEMATAP schemaTAP_SCHEMA.schemasList of schemasschema_nameFully qualified schema nameVARCHARdescriptionBrief description of schemaVARCHARutypeUTYPE if schema corresponds to a data modelVARCHARidFor internal purposesINTEGERTAP_SCHEMA.tablesList of tablesschema_nameFully qualified schema nameVARCHARtable_nameFully qualified table nameVARCHARtable_typeOne of: table or viewVARCHARdescriptionBrief description of tableVARCHARutypeUTYPE if table corresponds to a data modelVARCHARidFor internal purposesINTEGERTAP_SCHEMA.schemasschema_nameschema_nameTAP_SCHEMA.columnsList of columnstable_nameFully qualified table nameVARCHARcolumn_nameColumn nameVARCHARdescriptionBrief description of columnVARCHARunitUnit in VO std formatVARCHARucdUCD of column if anyVARCHARutypeUtypeVARCHARdatatypeADQL datatype as in section 2.5VARCHAR"size"Length of variable length datatypesINTEGERprincipalA principal column (1 true, 0 false)INTEGERindexedAn indexed column (1 true, 0 false)INTEGERstdA std column (1 true, 0 false)INTEGERidFor internal purposesINTEGERxtypeExtended ADQL data typeVARCHARTAP_SCHEMA.tablestable_nametable_nameTAP_SCHEMA.keysList of keyskey_idUnique key descriptorVARCHARfrom_tableFully qualified table nameVARCHARtarget_tableFully qualified table nameVARCHARdescriptionDescription of this keyVARCHARutypeUtype of this keyVARCHARidFor internal purposesINTEGERTAP_SCHEMA.tablesfrom_tabletable_nametarget_tabletable_nameTAP_SCHEMA.key_columnsList of key columnskey_idKey identifier from keys tableVARCHARfrom_columnKey column name in the from_tableVARCHARtarget_columnKey column name in the target_tableVARCHARidFor internal purposesINTEGERTAP_SCHEMA.columnsfrom_columncolumn_nametarget_columncolumn_nameTAP_SCHEMA.keyskey_idkey_idcsc21Chandra Source Catalog version 2.1csc21.coneCone search viewnameSource name in the format '2CXO Jhhmmss.s{+|-}ddmmss[X]'ID_MAINVARCHARprincipalindexedraSource position, ICRS right ascensiondegPOS_EQ_RA_MAINDOUBLEprincipalindexeddecSource position, ICRS declinationdegPOS_EQ_DEC_MAINDOUBLEprincipalindexederr_ellipse_r0Major radius of the 95% confidence level position error ellipsearcsecDOUBLEprincipalerr_ellipse_r1Minor radius of the 95% confidence level position error ellipsearcsecDOUBLEerr_ellipse_angPosition angle (ref. local true north) of the major axis of the 95% confidence level error ellipsedegDOUBLEgal_bSource position, Galactic latitude (equinox J2000.0, epoch J2000.0)degpos.galactic.latDOUBLEgal_lSource position, Galactic longitude (equinox J2000.0, epoch J2000.0)degpos.galactic.lonDOUBLEextent_flagSource is extended, or deconvolved source extent is inconsistent with a point source at the 90% confidence level in one or more observations and energy bandsBOOLEANconf_flagSource may be confused (source and/or background regions overlap in one or more contributing stacked observations)BOOLEANprincipalpileup_flagACIS pile-up fraction exceeds ~ 10% in all observations; source properties may be affectedBOOLEANvar_flagSource displays flux variability within one or more observations, or between observations, in one or more energy bandsBOOLEANstreak_src_flagSource is located on an ACIS readout streak in all observations; source properties may be affectedBOOLEANsat_src_flagSource is saturated in all observations; source properties are unreliableBOOLEANprincipalman_add_flagSource was manually added in the catalog via human reviewBOOLEANman_inc_flagSource was manually included in the catalog via human review (detection was rejected by automated criteria)BOOLEANman_reg_flagSource region parameters (dimensions, initial guess position input to the Maximum Likelihood Estimator fit) were manually modified via human reviewBOOLEANman_match_flagSource detections were manually matched between overlapping stacked observations via human reviewBOOLEANman_pos_flagBest fit source position was manually modified via human reviewBOOLEANvar_inter_hard_flagSource hardness ratios are statistically inconsistent between two or more observationsBOOLEANmajor_axis_b1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_h1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_m1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_s1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_u1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_w1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_b1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_h1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_m1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_s1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_lolim_u1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_lolim_w1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_b1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_h1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_m1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_s1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_hilim_u1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_hilim_w1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_b1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_h1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_m1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_s1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_u1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_w1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_b1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_h1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_m1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_s1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_lolim_u1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_lolim_w1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_b1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_h1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_m1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_s1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_hilim_u1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_hilim_w1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpos_angle_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpos_angle_lolim_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_lolim_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_lolim_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_lolim_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_lolim_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_lolim_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpos_angle_hilim_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_hilim_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_hilim_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_hilim_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_hilim_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_hilim_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEsrc_area_bArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS broad (0.5-7.0 keV) energy bandarcsec**2DOUBLEsrc_area_hArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS hard (2.0-7.0 keV) energy bandarcsec**2DOUBLEsrc_area_mArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS medium (1.2-2.0 keV) energy bandarcsec**2DOUBLEsrc_area_sArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS soft (0.5-1.2 keV) energy bandarcsec**2DOUBLEsrc_area_uArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsec**2DOUBLEsrc_area_wArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; HRC wide (~0.1-10.0 keV) energy bandarcsec**2DOUBLEphot_nsrcsNumber of sources fit simultaneously to compute aperture photometry quantitiesINTEGERphotflux_aper_bAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISphoton/s/cm**2DOUBLEphotflux_aper_hAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISphoton/s/cm**2DOUBLEphotflux_aper_mAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISphoton/s/cm**2DOUBLEphotflux_aper_sAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISphoton/s/cm**2DOUBLEphotflux_aper_uAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISphoton/s/cm**2DOUBLEphotflux_aper_wAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC wphoton/s/cm**2DOUBLEphotflux_aper_lolim_bAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_lolim_hAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_lolim_mAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_lolim_sAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_lolim_uAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_lolim_wAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_hilim_bAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper_hilim_hAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper_hilim_mAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper_hilim_sAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper_hilim_uAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper_hilim_wAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper90_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS brphoton/s/cm**2DOUBLEphotflux_aper90_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS haphoton/s/cm**2DOUBLEphotflux_aper90_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS mephoton/s/cm**2DOUBLEphotflux_aper90_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS sophoton/s/cm**2DOUBLEphotflux_aper90_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS ulphoton/s/cm**2DOUBLEphotflux_aper90_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC widphoton/s/cm**2DOUBLEphotflux_aper90_lolim_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_lolim_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_lolim_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_lolim_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_lolim_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_lolim_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_hilim_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEphotflux_aper90_hilim_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEphotflux_aper90_hilim_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEphotflux_aper90_hilim_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEphotflux_aper90_hilim_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEphotflux_aper90_hilim_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEflux_aper_bAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISerg/s/cm**2DOUBLEprincipalflux_aper_hAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISerg/s/cm**2DOUBLEflux_aper_mAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISerg/s/cm**2DOUBLEflux_aper_sAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISerg/s/cm**2DOUBLEflux_aper_uAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISerg/s/cm**2DOUBLEflux_aper_wAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC werg/s/cm**2DOUBLEprincipalflux_aper_lolim_bAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEprincipalflux_aper_lolim_hAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEflux_aper_lolim_mAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEflux_aper_lolim_sAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEflux_aper_lolim_uAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEflux_aper_lolim_wAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEprincipalflux_aper_hilim_bAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEprincipalflux_aper_hilim_hAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEflux_aper_hilim_mAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEflux_aper_hilim_sAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEflux_aper_hilim_uAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEflux_aper_hilim_wAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEprincipalflux_aper90_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS brerg/s/cm**2DOUBLEflux_aper90_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS haerg/s/cm**2DOUBLEflux_aper90_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS meerg/s/cm**2DOUBLEflux_aper90_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS soerg/s/cm**2DOUBLEflux_aper90_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS ulerg/s/cm**2DOUBLEflux_aper90_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC widerg/s/cm**2DOUBLEflux_aper90_lolim_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_lolim_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_lolim_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_lolim_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_lolim_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_lolim_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_hilim_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEflux_aper90_hilim_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEflux_aper90_hilim_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEflux_aper90_hilim_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEflux_aper90_hilim_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEflux_aper90_hilim_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEphotflux_aper_avg_bAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_mAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_sAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_uAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_wAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_bAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_hAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_mAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_sAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_uAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_wAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_bAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_hAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_mAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_sAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_uAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_wAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEflux_aper_avg_bAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_mAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_sAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_uAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_wAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_bAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_hAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_mAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_sAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_uAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_wAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_bAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_hAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_mAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_sAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_uAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_wAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_bSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_mSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_sSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_uSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_wSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_bSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_mSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_sSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_uSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_wSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_bSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_mSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_sSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_uSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_wSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_bSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_mSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_sSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_uSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_wSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLElikelihoodHighest detection log likelihood across all stacked observations and energy bandsDOUBLElikelihood_classHighest detection likelihood classification across all stacked observations and energy bandsVARCHARsignificanceHighest flux significance (S/N) across all stacked observations and energy bandsDOUBLEprincipalflux_powlawNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_powlaw_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_powlaw_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEpowlaw_gammaPhoton index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_gamma_lolimPhoton index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEpowlaw_gamma_hilimPhoton index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)DOUBLEpowlaw_gamma_rhatPhoton index convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_nhN_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEpowlaw_nh_lolimN_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEpowlaw_nh_hilimN_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEpowlaw_nh_rhatN_H column density convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_amplAmplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_ampl_lolimAmplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEpowlaw_ampl_hilimAmplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEpowlaw_ampl_rhatAmplitude convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_statchi-square statistic per degree of freedom of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEflux_bbNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_bb_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_bb_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEbb_ktTemperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumkeVDOUBLEbb_kt_lolimTemperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)keVDOUBLEbb_kt_hilimTemperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)keVDOUBLEbb_kt_rhatTemperature (kT) convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_nhN_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEbb_nh_lolimN_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEbb_nh_hilimN_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEbb_nh_rhatN_H column density convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_amplAmplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_ampl_lolimAmplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEbb_ampl_hilimAmplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEbb_ampl_rhatAmplitude convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_statchi-square statistic per degree of freedom of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEflux_bremsNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_brems_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_brems_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEbrems_ktTemperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumkeVDOUBLEbrems_kt_lolimTemperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)keVDOUBLEbrems_kt_hilimTemperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)keVDOUBLEbrems_kt_rhatTemperature (kT) convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_nhN_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEbrems_nh_lolimN_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEbrems_nh_hilimN_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEbrems_nh_rhatN_H column density convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_normAmplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_norm_lolimAmplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEbrems_norm_hilimAmplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEbrems_norm_rhatAmplitude convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_statchi-square statistic per degree of freedom of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEflux_apecNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_apec_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_apec_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEapec_ktTemperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumkeVDOUBLEapec_kt_lolimTemperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)keVDOUBLEapec_kt_hilimTemperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)keVDOUBLEapec_kt_rhatTemperature (kT) convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_abundAbundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_abund_lolimAbundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEapec_abund_hilimAbundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)DOUBLEapec_abund_rhatAbundance convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_zRedshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_z_lolimRedshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEapec_z_hilimRedshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)DOUBLEapec_z_rhatRedshift convergence criterion Redshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_nhN_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEapec_nh_lolimN_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEapec_nh_hilimN_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEapec_nh_rhatN_H column density convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_normAmplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_norm_lolimAmplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEapec_norm_hilimAmplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEapec_norm_rhatAmplitude convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_statchi-square statistic per degree of freedom of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEnh_galGalactic N_H column density in direction of source10**20/cm**2DOUBLEhard_hmACIS hard - medium (1.2-2.0 keV) energy band hardness ratioDOUBLEhard_hm_lolimACIS hard - medium (1.2-2.0 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_hm_hilimACIS hard - medium (1.2-2.0 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEvar_inter_hard_prob_hmInter-observation ACIS hard - medium (1.2-2.0 keV) energy band hardness ratio variability probabilityDOUBLEvar_inter_hard_sigma_hmInter-observation ACIS hard - medium (1.2-2.0 keV) energy band hardness ratio variability standard deviationDOUBLEhard_hsACIS hard - soft (0.5-1.2 keV) energy band hardness ratioDOUBLEhard_hs_lolimACIS hard - soft (0.5-1.2 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_hs_hilimACIS hard - soft (0.5-1.2 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEvar_inter_hard_prob_hsInter-observation ACIS hard - soft (0.5-1.2 keV) energy band hardness ratio variability probabilityDOUBLEvar_inter_hard_sigma_hsInter-observation ACIS hard - soft (0.5-1.2 keV) energy band hardness ratio variability standard deviationDOUBLEhard_msACIS medium - soft (0.5-1.2 keV) energy band hardness ratioDOUBLEhard_ms_lolimACIS medium - soft (0.5-1.2 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_ms_hilimACIS medium - soft (0.5-1.2 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEvar_inter_hard_prob_msInter-observation ACIS medium - soft (0.5-1.2 keV) energy band hardness ratio variability probabilityDOUBLEvar_inter_hard_sigma_msInter-observation ACIS medium - soft (0.5-1.2 keV) energy band hardness ratio variability standard deviationDOUBLEks_intra_prob_bIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEks_intra_prob_hIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEks_intra_prob_mIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEks_intra_prob_sIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEks_intra_prob_uIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEks_intra_prob_wIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEkp_intra_prob_bIntra-observation Kuiper's test variability probability (highest value across all observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEkp_intra_prob_hIntra-observation Kuiper's test variability probability (highest value across all observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEkp_intra_prob_mIntra-observation Kuiper's test variability probability (highest value across all observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEkp_intra_prob_sIntra-observation Kuiper's test variability probability (highest value across all observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEkp_intra_prob_uIntra-observation Kuiper's test variability probability (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEkp_intra_prob_wIntra-observation Kuiper's test variability probability (highest value across all observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEvar_intra_prob_bIntra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEvar_intra_prob_hIntra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEvar_intra_prob_mIntra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEvar_intra_prob_sIntra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEvar_intra_prob_uIntra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEvar_intra_prob_wIntra-observation Gregory-Loredo variability probability (highest value across all observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEvar_intra_index_bIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS broad (0.5-7.0 keV) energy bandINTEGERvar_intra_index_hIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS hard (2.0-7.0 keV) energy bandINTEGERvar_intra_index_mIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS medium (1.2-2.0 keV) energy bandINTEGERvar_intra_index_sIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS soft (0.5-1.2 keV) energy bandINTEGERvar_intra_index_uIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy bandINTEGERvar_intra_index_wIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); HRC wide (~0.1-10.0 keV) energy bandINTEGERvar_inter_index_bInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS broad (0.5-7.0 keV) energy bandINTEGERvar_inter_index_hInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS hard (2.0-7.0 keV) energy bandINTEGERvar_inter_index_mInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS medium (1.2-2.0 keV) energy bandINTEGERvar_inter_index_sInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS soft (0.5-1.2 keV) energy bandINTEGERvar_inter_index_uInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS ultrasoft (0.2-0.5 keV) energy bandINTEGERvar_inter_index_wInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; HRC wide (~0.1-10.0 keV) energy bandINTEGERvar_inter_prob_bInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS broad (0.5-7.0 keV) energy bandDOUBLEvar_inter_prob_hInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS hard (2.0-7.0 keV) energy bandDOUBLEvar_inter_prob_mInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS medium (1.2-2.0 keV) energy bandDOUBLEvar_inter_prob_sInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS soft (0.5-1.2 keV) energy bandDOUBLEvar_inter_prob_uInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEvar_inter_prob_wInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; HRC wide (~0.1-10.0 keV) energy bandDOUBLEvar_inter_sigma_bInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_hInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_mInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_sInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_uInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_wInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEdither_warning_flagHighest statistically significant peak in the power spectrum of the source region count rate occurs at the dither frequency or at a beat frequency of the dither frequency in one or more observationsBOOLEANacis_numTotal number of ACIS imaging observations contributing to the Master Sources Table record of the sourceINTEGERacis_hetg_numTotal number of ACIS/HETG observations contributing to the Master Sources Table record of the sourceINTEGERacis_letg_numTotal number of ACIS/LETG observations contributing to the Master Sources Table record of the sourceINTEGERacis_timeTotal exposure time (seconds of good time) for all ACIS imaging observations contributing to the Master Sources Table record of the sourcesDOUBLEacis_hetg_timeTotal exposure time (seconds of good time) for all ACIS/HETG observations contributing to the Master Sources Table record of the sourcesDOUBLEacis_letg_timeTotal exposure time (seconds of good time) for all ACIS/LETG observations contributing to the Master Sources Table record of the sourcesDOUBLEhrc_numTotal number of HRC imaging observations contributing to the Master Sources Table record of the sourceINTEGERhrc_hetg_numTotal number of HRC/HETG observations contributing to the Master Sources Table record of the sourceINTEGERhrc_letg_numTotal number of HRC/LETG observations contributing to the Master Sources Table record of the sourceINTEGERhrc_timeTotal exposure time (seconds of good time) for all HRC imaging observations contributing to the Master Sources Table record of the sourcesDOUBLEhrc_hetg_timeTotal exposure time (seconds of good time) for all HRC/HETG observations contributing to the Master Sources Table record of the sourcesDOUBLEhrc_letg_timeTotal exposure time (seconds of good time) for all HRC/LETG observations contributing to the Master Sources Table record of the sourcesDOUBLEcsc21.master_sourceMaster SourcesnameSource name in the format '2CXO Jhhmmss.s{+|-}ddmmss[X]'VARCHARprincipalindexedraSource position, ICRS right ascensiondegpos.eq.ra;meta.mainDOUBLEprincipalindexeddecSource position, ICRS declinationdegpos.eq.dec;meta.mainDOUBLEprincipalindexederr_ellipse_r0Major radius of the 95% confidence level position error ellipsearcsecDOUBLEprincipalerr_ellipse_r1Minor radius of the 95% confidence level position error ellipsearcsecDOUBLEerr_ellipse_angPosition angle (ref. local true north) of the major axis of the 95% confidence level error ellipsedegDOUBLEgal_bSource position, Galactic latitude (equinox J2000.0, epoch J2000.0)degpos.galactic.latDOUBLEgal_lSource position, Galactic longitude (equinox J2000.0, epoch J2000.0)degpos.galactic.lonDOUBLEextent_flagSource is extended, or deconvolved source extent is inconsistent with a point source at the 90% confidence level in one or more observations and energy bandsBOOLEANconf_flagSource may be confused (source and/or background regions overlap in one or more contributing stacked observations)BOOLEANprincipalpileup_flagACIS pile-up fraction exceeds ~ 10% in all observations; source properties may be affectedBOOLEANvar_flagSource displays flux variability within one or more observations, or between observations, in one or more energy bandsBOOLEANstreak_src_flagSource is located on an ACIS readout streak in all observations; source properties may be affectedBOOLEANsat_src_flagSource is saturated in all observations; source properties are unreliableBOOLEANprincipalman_add_flagSource was manually added in the catalog via human reviewBOOLEANman_inc_flagSource was manually included in the catalog via human review (detection was rejected by automated criteria)BOOLEANman_reg_flagSource region parameters (dimensions, initial guess position input to the Maximum Likelihood Estimator fit) were manually modified via human reviewBOOLEANman_match_flagSource detections were manually matched between overlapping stacked observations via human reviewBOOLEANman_pos_flagBest fit source position was manually modified via human reviewBOOLEANvar_inter_hard_flagSource hardness ratios are statistically inconsistent between two or more observationsBOOLEANmajor_axis_b1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_h1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_m1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_s1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_u1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_w1 sigma radius along the major axis of the ellipse defining the deconvolved source extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_b1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_h1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_m1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_s1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_lolim_u1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_lolim_w1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_b1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_h1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_m1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_s1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_hilim_u1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_hilim_w1 sigma radius along the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_b1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_h1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_m1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_s1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_u1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_w1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_b1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_h1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_m1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_s1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_lolim_u1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_lolim_w1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_b1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_h1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_m1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_s1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_hilim_u1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_hilim_w1 sigma radius along the minor axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpos_angle_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent; HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpos_angle_lolim_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_lolim_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_lolim_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_lolim_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_lolim_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_lolim_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpos_angle_hilim_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_hilim_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_hilim_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_hilim_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_hilim_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_hilim_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved source extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEsrc_area_bArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS broad (0.5-7.0 keV) energy bandarcsec**2DOUBLEsrc_area_hArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS hard (2.0-7.0 keV) energy bandarcsec**2DOUBLEsrc_area_mArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS medium (1.2-2.0 keV) energy bandarcsec**2DOUBLEsrc_area_sArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS soft (0.5-1.2 keV) energy bandarcsec**2DOUBLEsrc_area_uArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsec**2DOUBLEsrc_area_wArea of the deconvolved source extent ellipse, or area of the source polygon for extended sources; HRC wide (~0.1-10.0 keV) energy bandarcsec**2DOUBLEphot_nsrcsNumber of sources fit simultaneously to compute aperture photometry quantitiesINTEGERphotflux_aper_bAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISphoton/s/cm**2DOUBLEphotflux_aper_hAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISphoton/s/cm**2DOUBLEphotflux_aper_mAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISphoton/s/cm**2DOUBLEphotflux_aper_sAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISphoton/s/cm**2DOUBLEphotflux_aper_uAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISphoton/s/cm**2DOUBLEphotflux_aper_wAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC wphoton/s/cm**2DOUBLEphotflux_aper_lolim_bAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_lolim_hAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_lolim_mAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_lolim_sAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_lolim_uAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_lolim_wAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lphoton/s/cm**2DOUBLEphotflux_aper_hilim_bAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper_hilim_hAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper_hilim_mAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper_hilim_sAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper_hilim_uAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper_hilim_wAperture-corrected net photon flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uphoton/s/cm**2DOUBLEphotflux_aper90_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS brphoton/s/cm**2DOUBLEphotflux_aper90_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS haphoton/s/cm**2DOUBLEphotflux_aper90_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS mephoton/s/cm**2DOUBLEphotflux_aper90_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS sophoton/s/cm**2DOUBLEphotflux_aper90_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS ulphoton/s/cm**2DOUBLEphotflux_aper90_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC widphoton/s/cm**2DOUBLEphotflux_aper90_lolim_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_lolim_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_lolim_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_lolim_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_lolim_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_lolim_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowphoton/s/cm**2DOUBLEphotflux_aper90_hilim_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEphotflux_aper90_hilim_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEphotflux_aper90_hilim_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEphotflux_aper90_hilim_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEphotflux_aper90_hilim_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEphotflux_aper90_hilim_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uppphoton/s/cm**2DOUBLEflux_aper_bAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISerg/s/cm**2DOUBLEprincipalflux_aper_hAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISerg/s/cm**2DOUBLEflux_aper_mAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISerg/s/cm**2DOUBLEflux_aper_sAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISerg/s/cm**2DOUBLEflux_aper_uAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACISerg/s/cm**2DOUBLEflux_aper_wAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC werg/s/cm**2DOUBLEprincipalflux_aper_lolim_bAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEprincipalflux_aper_lolim_hAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEflux_aper_lolim_mAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEflux_aper_lolim_sAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEflux_aper_lolim_uAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEflux_aper_lolim_wAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lerg/s/cm**2DOUBLEprincipalflux_aper_hilim_bAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEprincipalflux_aper_hilim_hAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEflux_aper_hilim_mAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEflux_aper_hilim_sAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEflux_aper_hilim_uAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEflux_aper_hilim_wAperture-corrected net energy flux inferred from the source region aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% uerg/s/cm**2DOUBLEprincipalflux_aper90_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS brerg/s/cm**2DOUBLEflux_aper90_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS haerg/s/cm**2DOUBLEflux_aper90_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS meerg/s/cm**2DOUBLEflux_aper90_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS soerg/s/cm**2DOUBLEflux_aper90_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; ACIS ulerg/s/cm**2DOUBLEflux_aper90_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events; HRC widerg/s/cm**2DOUBLEflux_aper90_lolim_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_lolim_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_lolim_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_lolim_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_lolim_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_lolim_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% lowerg/s/cm**2DOUBLEflux_aper90_hilim_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEflux_aper90_hilim_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEflux_aper90_hilim_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEflux_aper90_hilim_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEflux_aper90_hilim_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEflux_aper90_hilim_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, best estimate derived from the longest block of a multi-band, flux-ordered Bayesian Block analysis of the contributing observations, and calculated by counting X-ray events (68% upperg/s/cm**2DOUBLEphotflux_aper_avg_bAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_mAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_sAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_uAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_wAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_bAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_hAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_mAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_sAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_uAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_lolim_wAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_bAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_hAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_mAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_sAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_uAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_avg_hilim_wAperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_lolim_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_bAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_hAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_mAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_sAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_uAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_avg_hilim_wAperture-corrected net photon flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEflux_aper_avg_bAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_mAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_sAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_uAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_wAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_bAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_hAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_mAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_sAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_uAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_lolim_wAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_bAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_hAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_mAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_sAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_uAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_avg_hilim_wAperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_lolim_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_bAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_hAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_mAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_sAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_uAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_avg_hilim_wAperture-corrected net energy flux inferred from the PSF 90% ECF aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_bSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_mSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_sSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_uSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_wSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_bSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_mSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_sSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_uSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_wSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_bSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_mSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_sSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_uSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_wSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_bSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_mSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_sSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_uSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_wSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLElikelihoodHighest detection log likelihood across all stacked observations and energy bandsDOUBLElikelihood_classHighest detection likelihood classification across all stacked observations and energy bandsVARCHARsignificanceHighest flux significance (S/N) across all stacked observations and energy bandsDOUBLEprincipalflux_powlawNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_powlaw_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_powlaw_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEpowlaw_gammaPhoton index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_gamma_lolimPhoton index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEpowlaw_gamma_hilimPhoton index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)DOUBLEpowlaw_gamma_rhatPhoton index convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_nhN_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEpowlaw_nh_lolimN_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEpowlaw_nh_hilimN_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEpowlaw_nh_rhatN_H column density convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_amplAmplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_ampl_lolimAmplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEpowlaw_ampl_hilimAmplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEpowlaw_ampl_rhatAmplitude convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_statchi-square statistic per degree of freedom of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEflux_bbNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_bb_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_bb_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEbb_ktTemperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumkeVDOUBLEbb_kt_lolimTemperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)keVDOUBLEbb_kt_hilimTemperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)keVDOUBLEbb_kt_rhatTemperature (kT) convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_nhN_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEbb_nh_lolimN_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEbb_nh_hilimN_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEbb_nh_rhatN_H column density convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_amplAmplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_ampl_lolimAmplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEbb_ampl_hilimAmplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEbb_ampl_rhatAmplitude convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_statchi-square statistic per degree of freedom of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEflux_bremsNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_brems_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_brems_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEbrems_ktTemperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumkeVDOUBLEbrems_kt_lolimTemperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)keVDOUBLEbrems_kt_hilimTemperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)keVDOUBLEbrems_kt_rhatTemperature (kT) convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_nhN_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEbrems_nh_lolimN_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEbrems_nh_hilimN_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEbrems_nh_rhatN_H column density convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_normAmplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_norm_lolimAmplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEbrems_norm_hilimAmplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEbrems_norm_rhatAmplitude convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_statchi-square statistic per degree of freedom of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEflux_apecNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_apec_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_apec_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEapec_ktTemperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumkeVDOUBLEapec_kt_lolimTemperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)keVDOUBLEapec_kt_hilimTemperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)keVDOUBLEapec_kt_rhatTemperature (kT) convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_abundAbundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_abund_lolimAbundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEapec_abund_hilimAbundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)DOUBLEapec_abund_rhatAbundance convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_zRedshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_z_lolimRedshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEapec_z_hilimRedshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)DOUBLEapec_z_rhatRedshift convergence criterion Redshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_nhN_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEapec_nh_lolimN_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEapec_nh_hilimN_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEapec_nh_rhatN_H column density convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_normAmplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_norm_lolimAmplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEapec_norm_hilimAmplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEapec_norm_rhatAmplitude convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_statchi-square statistic per degree of freedom of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEnh_galGalactic N_H column density in direction of source10**20/cm**2DOUBLEhard_hmACIS hard - medium (1.2-2.0 keV) energy band hardness ratioDOUBLEhard_hm_lolimACIS hard - medium (1.2-2.0 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_hm_hilimACIS hard - medium (1.2-2.0 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEvar_inter_hard_prob_hmInter-observation ACIS hard - medium (1.2-2.0 keV) energy band hardness ratio variability probabilityDOUBLEvar_inter_hard_sigma_hmInter-observation ACIS hard - medium (1.2-2.0 keV) energy band hardness ratio variability standard deviationDOUBLEhard_hsACIS hard - soft (0.5-1.2 keV) energy band hardness ratioDOUBLEhard_hs_lolimACIS hard - soft (0.5-1.2 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_hs_hilimACIS hard - soft (0.5-1.2 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEvar_inter_hard_prob_hsInter-observation ACIS hard - soft (0.5-1.2 keV) energy band hardness ratio variability probabilityDOUBLEvar_inter_hard_sigma_hsInter-observation ACIS hard - soft (0.5-1.2 keV) energy band hardness ratio variability standard deviationDOUBLEhard_msACIS medium - soft (0.5-1.2 keV) energy band hardness ratioDOUBLEhard_ms_lolimACIS medium - soft (0.5-1.2 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_ms_hilimACIS medium - soft (0.5-1.2 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEvar_inter_hard_prob_msInter-observation ACIS medium - soft (0.5-1.2 keV) energy band hardness ratio variability probabilityDOUBLEvar_inter_hard_sigma_msInter-observation ACIS medium - soft (0.5-1.2 keV) energy band hardness ratio variability standard deviationDOUBLEks_intra_prob_bIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEks_intra_prob_hIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEks_intra_prob_mIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEks_intra_prob_sIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEks_intra_prob_uIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEks_intra_prob_wIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEkp_intra_prob_bIntra-observation Kuiper's test variability probability (highest value across all observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEkp_intra_prob_hIntra-observation Kuiper's test variability probability (highest value across all observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEkp_intra_prob_mIntra-observation Kuiper's test variability probability (highest value across all observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEkp_intra_prob_sIntra-observation Kuiper's test variability probability (highest value across all observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEkp_intra_prob_uIntra-observation Kuiper's test variability probability (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEkp_intra_prob_wIntra-observation Kuiper's test variability probability (highest value across all observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEvar_intra_prob_bIntra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEvar_intra_prob_hIntra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEvar_intra_prob_mIntra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEvar_intra_prob_sIntra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEvar_intra_prob_uIntra-observation Gregory-Loredo variability probability (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEvar_intra_prob_wIntra-observation Gregory-Loredo variability probability (highest value across all observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEvar_intra_index_bIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS broad (0.5-7.0 keV) energy bandINTEGERvar_intra_index_hIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS hard (2.0-7.0 keV) energy bandINTEGERvar_intra_index_mIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS medium (1.2-2.0 keV) energy bandINTEGERvar_intra_index_sIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS soft (0.5-1.2 keV) energy bandINTEGERvar_intra_index_uIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy bandINTEGERvar_intra_index_wIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all observations); HRC wide (~0.1-10.0 keV) energy bandINTEGERvar_inter_index_bInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS broad (0.5-7.0 keV) energy bandINTEGERvar_inter_index_hInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS hard (2.0-7.0 keV) energy bandINTEGERvar_inter_index_mInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS medium (1.2-2.0 keV) energy bandINTEGERvar_inter_index_sInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS soft (0.5-1.2 keV) energy bandINTEGERvar_inter_index_uInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS ultrasoft (0.2-0.5 keV) energy bandINTEGERvar_inter_index_wInter-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; HRC wide (~0.1-10.0 keV) energy bandINTEGERvar_inter_prob_bInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS broad (0.5-7.0 keV) energy bandDOUBLEvar_inter_prob_hInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS hard (2.0-7.0 keV) energy bandDOUBLEvar_inter_prob_mInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS medium (1.2-2.0 keV) energy bandDOUBLEvar_inter_prob_sInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS soft (0.5-1.2 keV) energy bandDOUBLEvar_inter_prob_uInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEvar_inter_prob_wInter-observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; HRC wide (~0.1-10.0 keV) energy bandDOUBLEvar_inter_sigma_bInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_hInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_mInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_sInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_uInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_wInter-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEdither_warning_flagHighest statistically significant peak in the power spectrum of the source region count rate occurs at the dither frequency or at a beat frequency of the dither frequency in one or more observationsBOOLEANacis_numTotal number of ACIS imaging observations contributing to the Master Sources Table record of the sourceINTEGERacis_hetg_numTotal number of ACIS/HETG observations contributing to the Master Sources Table record of the sourceINTEGERacis_letg_numTotal number of ACIS/LETG observations contributing to the Master Sources Table record of the sourceINTEGERacis_timeTotal exposure time (seconds of good time) for all ACIS imaging observations contributing to the Master Sources Table record of the sourcesDOUBLEacis_hetg_timeTotal exposure time (seconds of good time) for all ACIS/HETG observations contributing to the Master Sources Table record of the sourcesDOUBLEacis_letg_timeTotal exposure time (seconds of good time) for all ACIS/LETG observations contributing to the Master Sources Table record of the sourcesDOUBLEhrc_numTotal number of HRC imaging observations contributing to the Master Sources Table record of the sourceINTEGERhrc_hetg_numTotal number of HRC/HETG observations contributing to the Master Sources Table record of the sourceINTEGERhrc_letg_numTotal number of HRC/LETG observations contributing to the Master Sources Table record of the sourceINTEGERhrc_timeTotal exposure time (seconds of good time) for all HRC imaging observations contributing to the Master Sources Table record of the sourcesDOUBLEhrc_hetg_timeTotal exposure time (seconds of good time) for all HRC/HETG observations contributing to the Master Sources Table record of the sourcesDOUBLEhrc_letg_timeTotal exposure time (seconds of good time) for all HRC/LETG observations contributing to the Master Sources Table record of the sourcesDOUBLEcsc21.stack_sourceStacked Observation Detectionsdetect_stack_idDetect stack identifier (designation of observation stack used for source detection) in the format '{acis|hrc}fJhhmmsss{+|-}ddmmss_nnn'VARCHARra_stackDetect stack tangent plane reference position, ICRS right ascensiondegpos.eq.raDOUBLEdec_stackDetect stack tangent plane reference position, ICRS declinationdegpos.eq.decDOUBLEinstrumentInstrument used for the stacked observations; 'ACIS' or 'HRC'VARCHARgratingTransmission grating used for the stacked observations; 'NONE', 'HETG', or 'LETGVARCHARascdsverSoftware version used to create the Level 3 detect stack event data fileVARCHARcaldbverCalibration database version used to calibrate the Level 3 detect stack event data fileVARCHARcrdateCreation date/time of the Level 3 detect stack event data file, UTCVARCHARregion_idDetection region identifier (component number)INTEGERprincipalraDetection position, ICRS Right Ascensiondegpos.eq.raDOUBLEprincipaldecDetection position, ICRS Declinationdegpos.eq.decDOUBLEprincipalerr_ellipse_r0Major radius of the 95% confidence level position error ellipsearcsecDOUBLEprincipalerr_ellipse_r1Minor radius of the 95% confidence level position error ellipsearcsecDOUBLEerr_ellipse_angPosition angle (ref. local true north) of the major axis of the 95% confidence level error ellipsedegDOUBLEtheta_meanMean source region aperture off-axis angle from all stacked observationsarcminDOUBLElikelihood_blog likelihood of the stacked-observation detection computed by the Maximum Likelihood Estimator fit to the photon counts distribution; ACIS broad (0.5-7.0 keV) energy bandDOUBLElikelihood_hlog likelihood of the stacked-observation detection computed by the Maximum Likelihood Estimator fit to the photon counts distribution; ACIS hard (2.0-7.0 keV) energy bandDOUBLElikelihood_mlog likelihood of the stacked-observation detection computed by the Maximum Likelihood Estimator fit to the photon counts distribution; ACIS medium (1.2-2.0 keV) energy bandDOUBLElikelihood_slog likelihood of the stacked-observation detection computed by the Maximum Likelihood Estimator fit to the photon counts distribution; ACIS soft (0.5-1.2 keV) energy bandDOUBLElikelihood_ulog likelihood of the stacked-observation detection computed by the Maximum Likelihood Estimator fit to the photon counts distribution; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLElikelihood_wlog likelihood of the stacked-observation detection computed by the Maximum Likelihood Estimator fit to the photon counts distribution; HRC wide (~0.1-10.0 keV) energy bandDOUBLElikelihood_classHighest detection likelihood classification across all energy bandsVARCHARdetect_significance_bSignificance of the stacked-observation detection computed by the stacked-observation detection algorithm; ACIS broad (0.5-7.0 keV) energy bandDOUBLEdetect_significance_hSignificance of the stacked-observation detection computed by the stacked-observation detection algorithm; ACIS hard (2.0-7.0 keV) energy bandDOUBLEdetect_significance_mSignificance of the stacked-observation detection computed by the stacked-observation detection algorithm; ACIS medium (1.2-2.0 keV) energy bandDOUBLEdetect_significance_sSignificance of the stacked-observation detection computed by the stacked-observation detection algorithm; ACIS soft (0.5-1.2 keV) energy bandDOUBLEdetect_significance_uSignificance of the stacked-observation detection computed by the stacked-observation detection algorithm; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEdetect_significance_wSignificance of the stacked-observation detection computed by the stacked-observation detection algorithm; HRC wide (~0.1-10.0 keV) energy bandDOUBLEflux_significance_bSignificance of the stacked-observation detection determined from the ratio of the stacked-observation detection flux to the estimated error in the local background; ACIS broad (0.5-7.0 keV) energy bandDOUBLEprincipalflux_significance_hSignificance of the stacked-observation detection determined from the ratio of the stacked-observation detection flux to the estimated error in the local background; ACIS hard (2.0-7.0 keV) energy bandDOUBLEflux_significance_mSignificance of the stacked-observation detection determined from the ratio of the stacked-observation detection flux to the estimated error in the local background; ACIS medium (1.2-2.0 keV) energy bandDOUBLEflux_significance_sSignificance of the stacked-observation detection determined from the ratio of the stacked-observation detection flux to the estimated error in the local background; ACIS soft (0.5-1.2 keV) energy bandDOUBLEflux_significance_uSignificance of the stacked-observation detection determined from the ratio of the stacked-observation detection flux to the estimated error in the local background; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEflux_significance_wSignificance of the stacked-observation detection determined from the ratio of the stacked-observation detection flux to the estimated error in the local background; HRC wide (~0.1-10.0 keV) energy bandDOUBLEprincipalextent_codeDetection is extended, or deconvolved compact detection extent is inconsistent with a point source at the 90% confidence level in one or more of the stacked observations and energy bands (bit encoded: 1, 2, 4, 8, 16, 32: deconvolved compact detection extenINTEGERconf_codeCompact detection may be confused (bit encoded: 1: background region overlaps another background region; 2: background region overlaps another source region; 4: source region overlaps another background region; 8: source region overlaps another source regiINTEGERprincipalpileup_flagACIS pile-up fraction exceeds ~ 10% in any stacked observation; detection properties may be affectedBOOLEANvar_flagDetection displays flux variability within one or more of the stacked observations, or between stacked observations, in one or more energy bandsBOOLEANedge_codeDetection position, or source or background region dithered off a detector boundary (chip pixel mask) during one or more of the stacked observations (bit encoded: 1: background region dithers off detector boundary; 2:source region dithers off detector bounINTEGERmulti_chip_codeSource position, or source or background region dithered multiple detector chips during one or more of the stacked observations (bit encoded: 1: background region dithers across 2 chips; 2: background region dithers across >2 chips; 4: source region ditherINTEGERstreak_src_flagDetection is located on an ACIS readout streak in all stacked observations; detection properties may be affectedBOOLEANsat_src_flagDetection is saturated in all stacked observations; detection properties are unreliableBOOLEANprincipalman_add_flagDetection was manually added in the catalog via human reviewBOOLEANman_inc_flagDetection was manually included in the catalog via human review (detection was rejected by automated criteria)BOOLEANman_reg_flagSource region parameters (dimensions, initial guess position input to the Maximum Likelihood Estimator fit) were manually modified via human reviewBOOLEANman_pos_flagBest fit detection position was manually modified via human reviewBOOLEANvar_inter_hard_flagDetection hardness ratios are statistically inconsistent between two or more of the stacked observationsBOOLEANra_aperCenter of the source region and background region apertures, ICRS right ascensiondegpos.eq.ra;instr.fovDOUBLEdec_aperCenter of the source region and background region apertures, ICRS declinationdegpos.eq.dec;instr.fovDOUBLEmjr_axis_aperSemi-major axis of the elliptical source region aperturearcsecDOUBLEmnr_axis_aperSemi-minor axis of the elliptical source region aperturearcsecDOUBLEpos_angle_aperPosition angle (ref. local true north) of the semi-major axis of the elliptical source region aperturedegDOUBLEmjr_axis1_aperbkgSemi-major axis of the inner ellipse of the annular background region aperturearcsecDOUBLEmnr_axis1_aperbkgSemi-minor axis of the inner ellipse of the annular background region aperturearcsecDOUBLEmjr_axis2_aperbkgSemi-major axis of the outer ellipse of the annular background region aperturearcsecDOUBLEmnr_axis2_aperbkgSemi-minor axis of the outer ellipse of the annular background region aperturearcsecDOUBLEpos_angle_aperbkgPosition angle (ref. local true north) of the semi-major axes of the annular background region aperturedegDOUBLEmajor_axis_b1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_h1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_m1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_s1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_u1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_w1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_b1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_h1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_m1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_s1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_lolim_u1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_lolim_w1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_b1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_h1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_m1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_s1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_hilim_u1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_hilim_w1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_b1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_h1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_m1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_s1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_u1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_w1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_b1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_h1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_m1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_s1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_lolim_u1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_lolim_w1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_b1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_h1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_m1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_s1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_hilim_u1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_hilim_w1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpos_angle_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpos_angle_lolim_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_lolim_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_lolim_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_lolim_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_lolim_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_lolim_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpos_angle_hilim_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_hilim_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_hilim_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_hilim_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_hilim_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_hilim_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEsrc_area_bArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; ACIS broad (0.5-7.0 keV) energy bandarcsec**2DOUBLEsrc_area_hArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; ACIS hard (2.0-7.0 keV) energy bandarcsec**2DOUBLEsrc_area_mArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; ACIS medium (1.2-2.0 keV) energy bandarcsec**2DOUBLEsrc_area_sArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; ACIS soft (0.5-1.2 keV) energy bandarcsec**2DOUBLEsrc_area_uArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsec**2DOUBLEsrc_area_wArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; HRC wide (~0.1-10.0 keV) energy bandarcsec**2DOUBLEphot_nsrcsNumber of detections fit simultaneously to compute aperture photometry quantitiesINTEGERsrc_cnts_aper_bAperture-corrected detection net counts inferred from the source region aperture; ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_hAperture-corrected detection net counts inferred from the source region aperture; ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_mAperture-corrected detection net counts inferred from the source region aperture; ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper_sAperture-corrected detection net counts inferred from the source region aperture; ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper_uAperture-corrected detection net counts inferred from the source region aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper_wAperture-corrected detection net counts inferred from the source region aperture; HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_bAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_hAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_mAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_sAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_uAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_wAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_bAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_hAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_mAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_sAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_uAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_wAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_bAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_hAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_mAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_sAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper90_uAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper90_wAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_bAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_hAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_mAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_sAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_uAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_wAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_bAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_hAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_mAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_sAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_uAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_wAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEsrc_rate_aper_bAperture-corrected detection net count rate inferred from the source region aperture; ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_hAperture-corrected detection net count rate inferred from the source region aperture; ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_mAperture-corrected detection net count rate inferred from the source region aperture; ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_sAperture-corrected detection net count rate inferred from the source region aperture; ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper_uAperture-corrected detection net count rate inferred from the source region aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper_wAperture-corrected detection net count rate inferred from the source region aperture; HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_bAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_hAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_mAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_sAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_uAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_wAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_bAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_hAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_mAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_sAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_uAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_wAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_bAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_mAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_sAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper90_uAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper90_wAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_bAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_hAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_mAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_sAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_uAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_wAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_bAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_hAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_mAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_sAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_uAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_wAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEphotflux_aper_bAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_mAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_sAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_uAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_wAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_bAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_hAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_mAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_sAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_uAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_wAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_bAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_hAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_mAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_sAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_uAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_wAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_bAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_mAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_sAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_uAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_wAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_bAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_hAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_mAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_sAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_uAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_wAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_bAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_hAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_mAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_sAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_uAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_wAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEflux_aper_bAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper_hAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_mAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_sAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_uAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_wAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper_lolim_bAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper_lolim_hAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_lolim_mAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_lolim_sAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_lolim_uAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_lolim_wAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper_hilim_bAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper_hilim_hAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_hilim_mAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_hilim_sAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_hilim_uAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_hilim_wAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper90_bAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_mAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_sAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_uAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_wAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_bAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_hAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_mAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_sAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_uAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_wAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_bAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_hAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_mAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_sAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_uAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_wAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEhard_hmACIS hard - medium (1.2-2.0 keV) energy band hardness ratioDOUBLEhard_hm_lolimACIS hard - medium (1.2-2.0 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_hm_hilimACIS hard - medium (1.2-2.0 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEvar_inter_hard_prob_hmInter-stacked-observation ACIS hard - medium (1.2-2.0 keV) energy band hardness ratio variability probabilityDOUBLEvar_inter_hard_sigma_hmInter-stacked-observation ACIS hard - medium (1.2-2.0 keV) energy band hardness ratio variability standard deviationDOUBLEhard_hsACIS hard - soft (0.5-1.2 keV) energy band hardness ratioDOUBLEhard_hs_lolimACIS hard - soft (0.5-1.2 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_hs_hilimACIS hard - soft (0.5-1.2 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEvar_inter_hard_prob_hsInter-stacked-observation ACIS hard - soft (0.5-1.2 keV) energy band hardness ratio variability probabilityDOUBLEvar_inter_hard_sigma_hsInter-stacked-observation ACIS hard - soft (0.5-1.2 keV) energy band hardness ratio variability standard deviationDOUBLEhard_msACIS medium - soft (0.5-1.2 keV) energy band hardness ratioDOUBLEhard_ms_lolimACIS medium - soft (0.5-1.2 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_ms_hilimACIS medium - soft (0.5-1.2 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEvar_inter_hard_prob_msInter-stacked-observation ACIS medium - soft (0.5-1.2 keV) energy band hardness ratio variability probabilityDOUBLEvar_inter_hard_sigma_msInter-stacked-observation ACIS medium - soft (0.5-1.2 keV) energy band hardness ratio variability standard deviationDOUBLEks_intra_prob_bIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEks_intra_prob_hIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEks_intra_prob_mIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEks_intra_prob_sIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEks_intra_prob_uIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEks_intra_prob_wIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEkp_intra_prob_bIntra-observation Kuiper's test variability probability (highest value across all stacked observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEkp_intra_prob_hIntra-observation Kuiper's test variability probability (highest value across all stacked observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEkp_intra_prob_mIntra-observation Kuiper's test variability probability (highest value across all stacked observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEkp_intra_prob_sIntra-observation Kuiper's test variability probability (highest value across all stacked observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEkp_intra_prob_uIntra-observation Kuiper's test variability probability (highest value across all stacked observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEkp_intra_prob_wIntra-observation Kuiper's test variability probability (highest value across all stacked observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEvar_intra_prob_bIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEvar_intra_prob_hIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEvar_intra_prob_mIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEvar_intra_prob_sIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEvar_intra_prob_uIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEvar_intra_prob_wIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEvar_intra_index_bIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); ACIS broad (0.5-7.0 keV) energy bandINTEGERvar_intra_index_hIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); ACIS hard (2.0-7.0 keV) energy bandINTEGERvar_intra_index_mIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); ACIS medium (1.2-2.0 keV) energy bandINTEGERvar_intra_index_sIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); ACIS soft (0.5-1.2 keV) energy bandINTEGERvar_intra_index_uIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); ACIS ultrasoft (0.2-0.5 keV) energy bandINTEGERvar_intra_index_wIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); HRC wide (~0.1-10.0 keV) energy bandINTEGERvar_inter_prob_bInter-stacked observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS broad (0.5-7.0 keV) energy bandDOUBLEvar_inter_prob_hInter-stacked observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS hard (2.0-7.0 keV) energy bandDOUBLEvar_inter_prob_mInter-stacked observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS medium (1.2-2.0 keV) energy bandDOUBLEvar_inter_prob_sInter-stacked observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS soft (0.5-1.2 keV) energy bandDOUBLEvar_inter_prob_uInter-stacked observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEvar_inter_prob_wInter-stacked observation variability probability, calculated from the chi^2 distribution of the photon fluxes of the individual observations; HRC wide (~0.1-10.0 keV) energy bandDOUBLEvar_inter_index_bInter-stacked-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS broad (0.5-7.0 keV) energy bandINTEGERvar_inter_index_hInter-stacked-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS hard (2.0-7.0 keV) energy bandINTEGERvar_inter_index_mInter-stacked-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS medium (1.2-2.0 keV) energy bandINTEGERvar_inter_index_sInter-stacked-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS soft (0.5-1.2 keV) energy bandINTEGERvar_inter_index_uInter-stacked-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; ACIS ultrasoft (0.2-0.5 keV) energy bandINTEGERvar_inter_index_wInter-stacked-observation variability index in the range [0, 10]: indicates whether the source region photon flux is constant between observations; HRC wide (~0.1-10.0 keV) energy bandINTEGERvar_inter_sigma_bInter-stacked-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_hInter-stacked-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_mInter-stacked-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_sInter-stacked-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_uInter-stacked-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEvar_inter_sigma_wInter-stacked-observation flux variability standard deviation; the spread of the individual observation photon fluxes about the error weighted mean; HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEdither_warning_flagHighest statistically significant peak in the power spectrum of the detection source region count rate occurs at the dither frequency or at a beat frequency of the dither frequency in one or more of the stacked observationsBOOLEANlivetimeEffective stacked observation exposure time at the location of the detection, after applying the good time intervals and the deadtime correction factorsDOUBLEprincipaldeltaxSKY coordinate system X translation correction required to co-align the observation stack astrometric frame with the Gaia-CRF3 realization of the ICRFarcsecDOUBLEdeltaySKY coordinate system Y translation correction required to co-align the observation stack astrometric frame with the Gaia-CRF3 realization of the ICRFarcsecDOUBLEdeltarotSKY coordinate system roll angle correction required to co-align the observation stack astrometric frame with the Gaia-CRF3 realization of the ICRFdegDOUBLEdscaleSKY coordinate system scale factor correction required to co-align the observation stack astrometric frame with the Gaia-CRF3 realization of the ICRFdegDOUBLEman_astrom_flagObservation stack astrometric transform was manually modified via human reviewBOOLEANcsc21.observation_sourcePer-Observation DetectionsobsidObservation identifierINTEGERprincipalobiObservation interval numberINTEGERprincipaltargnameObservation target name specified by observerVARCHARra_targTarget position specified by observer, ICRS right ascensiondegpos.eq.ra;obs.field;obs.paramDOUBLEdec_targTarget position specified by observer, ICRS declinationdegpos.eq.dec;obs.field;obs.paramDOUBLEra_pntMean spacecraft pointing during the observation, ICRS right ascensiondegpos.eq.ra;stat.mean;obs.fieldDOUBLEdec_pntMean spacecraft pointing during the observation, ICRS declinationdegpos.eq.dec;stat.mean;obs.fieldDOUBLEroll_pntMean spacecraft roll angle during the observationdegDOUBLEchipx_pntDetector (chip coordinates) Cartesian x position corresponding to (ra_pnt, dec_pnt)pixelDOUBLEchipy_pntDetector (chip coordinates) Cartesian y position corresponding to (ra_pnt, dec_pnt)pixelDOUBLEchip_id_pntDetector (chip coordinates) identifier used to define (chipx_pnt, chipy_pnt)INTEGERra_nomObservation tangent plane reference position, ICRS right ascensiondegmeta.ref;pos.eq.ra;obs.fieldDOUBLEdec_nomObservation tangent plane reference position, ICRS declinationdegmeta.ref;pos.eq.dec;obs.fieldDOUBLEroll_nomObservation tangent plane roll angle (used to determine tangent plane North)degDOUBLEsim_xSIM focus stage position during observationmmDOUBLEsim_zSIM translation stage position during observationmmDOUBLEdyMean aspect dy offset during observationmmDOUBLEdzMean aspect dz offset during observationmmDOUBLEdthetaMean aspect dtheta during observationdegDOUBLEdeltaxSKY coordinate system X translation correction required to co-align the observation astrometric frame within the observation stackarcsecDOUBLEdeltaySKY coordinate system Y translation correction required to co-align the observation astrometric frame within the observation stackarcsecDOUBLEdeltarotSKY coordinate system roll angle correction required to co-align co-align the observation astrometric frame within the observation stackdegDOUBLEdscaleSKY coordinate system scale factor correction required to co-align co-align the observation astrometric frame within the observation stackdegDOUBLEman_astrom_flagObservation astrometric transform was manually modified via human reviewBOOLEANgti_startStart time of valid observation data (MET: seconds since 1998 Jan 01 00:00:00 TT)sDOUBLEgti_stopStop time of valid observation data (MET: seconds since 1998 Jan 01 00:00:00 TT)sDOUBLEgti_elapseTotal elapsed time of the observation (gti_stop - gti_start)sDOUBLEgti_obsStart time of valid observation data (TT), ISO 8601 format (yyyy-mm-ddThh:mm:ss)VARCHARgti_endStop time of valid observation data (TT), ISO 8601 format (yyyy-mm-ddThh:mm:ss)VARCHARgti_mjd_obsMJD corresponding to start time of valid observation data (TT)DOUBLEmjd_refMJD corresponding to 0s METDOUBLEinstrumentInstrument used for the observation; 'ACIS' or 'HRC'VARCHARgratingTransmission grating used for the observation; 'NONE', 'HETG', or 'LETGVARCHARdatamodeInstrument data mode used for the observationVARCHARreadmodeACIS readout mode used for the observationVARCHARcycleACIS readout cycle for the observation, 'P' (primary) or 'S' (secondary) for alternating exposure (interleaved) mode observations, or 'P' for other ACIS modesVARCHARexptimeACIS CCD frame timesDOUBLEtiming_modeHRC precision timing modeBOOLEANascdsverSoftware version used to create the Level 3 observation event data fileVARCHARcaldbverCalibration database version used to calibrate the Level 3 observation event data fileVARCHARcrdateCreation date/time of the Level 3 observation event data file, UTCVARCHARaoChandra observing cycle in which the observation was scheduledINTEGERregion_idDetection region identifier (component number)INTEGERprincipalthetaPSF 90% ECF aperture off-axis anglearcminDOUBLEprincipalphiPSF 90% ECF aperture azimuthal angledegDOUBLEprincipalchipxDetector (chip coordinates) Cartesian x position corresponding to (theta, phi)pixelDOUBLEchipyDetector (chip coordinates) Cartesian y position corresponding to (theta, phi)pixelDOUBLEchip_idDetector (chip coordinates) identifier used to define (chipx, chipy)INTEGERlikelihood_bSignificance of the single-observation detection computed by the single-observation detection algorithm; ACIS broad (0.5-7.0 keV) energy bandDOUBLElikelihood_hSignificance of the single-observation detection computed by the single-observation detection algorithm; ACIS hard (2.0-7.0 keV) energy bandDOUBLElikelihood_mSignificance of the single-observation detection computed by the single-observation detection algorithm; ACIS medium (1.2-2.0 keV) energy bandDOUBLElikelihood_sSignificance of the single-observation detection computed by the single-observation detection algorithm; ACIS soft (0.5-1.2 keV) energy bandDOUBLElikelihood_uSignificance of the single-observation detection computed by the single-observation detection algorithm; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLElikelihood_wSignificance of the single-observation detection computed by the single-observation detection algorithm; HRC wide (~0.1-10.0 keV) energy bandDOUBLEflux_significance_bSignificance of the single-observation detection determined from the ratio of the single-observation detection flux to the estimated error in the local background; ACIS broad (0.5-7.0 keV) energy bandDOUBLEprincipalflux_significance_hSignificance of the single-observation detection determined from the ratio of the single-observation detection flux to the estimated error in the local background; ACIS hard (2.0-7.0 keV) energy bandDOUBLEflux_significance_mSignificance of the single-observation detection determined from the ratio of the single-observation detection flux to the estimated error in the local background; ACIS medium (1.2-2.0 keV) energy bandDOUBLEflux_significance_sSignificance of the single-observation detection determined from the ratio of the single-observation detection flux to the estimated error in the local background; ACIS soft (0.5-1.2 keV) energy bandDOUBLEflux_significance_uSignificance of the single-observation detection determined from the ratio of the single-observation detection flux to the estimated error in the local background; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEflux_significance_wSignificance of the single-observation detection determined from the ratio of the single-observation detection flux to the estimated error in the local background; HRC wide (~0.1-10.0 keV) energy bandDOUBLEprincipalextent_codeDetection is extended, or deconvolved compact detection extent is inconsistent with a point source at the 90% confidence level in one or more energy bands (bit encoded: 1, 2, 4, 8, 16, 32: deconvolved compact detection extent is not consistent with a pointINTEGERconf_codeCompact detection may be confused (bit encoded: 1: background region overlaps another background region; 2: background region overlaps another source region; 4: source region overlaps another background region; 8: source region overlaps another source regiINTEGERprincipalpileup_warningACIS pile-up fraction estimated from the coiunt rate of the brightest 3x3 pixel islandcount/pixel/frameDOUBLEvar_codeDetection displays flux variability in one or more energy bands (bit encoded: 1,2,4,8,16,32: intra-observation variability detected in the ACIS ultrasoft, soft, medium, hard, broad, or HRC wide (~0.1-10.0 keV) energy band, respectively)INTEGERedge_codeDetection position, or source or background region dithered off a detector boundary (chip pixel mask) during the observation (bit encoded: 1: background region dithers off detector boundary; 2:source region dithers off detector boundary; 4: detection positINTEGERmulti_chip_codeSource position, or source or background region dithered multiple detector chips during the observation (bit encoded: 1: background region dithers across 2 chips; 2: background region dithers across >2 chips; 4: source region dithers across 2 chips; 8: souINTEGERstreak_src_flagDetection is located on an ACIS readout streak; detection properties may be affectedBOOLEANsat_src_flagDetection is saturated; detection properties are unreliableBOOLEANprincipalarea_aperArea of the modified elliptical source region aperture (includes corrections for exclusion regions due to overlapping detections)arcsec**2DOUBLEarea_aperbkgArea of the modified annular background region aperture (includes corrections for exclusion regions due to overlapping detections)arcsec**2DOUBLEmjr_axis_raw_b1 sigma radius along the major axis of the ellipse defining the observed detection extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmjr_axis_raw_h1 sigma radius along the major axis of the ellipse defining the observed detection extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmjr_axis_raw_m1 sigma radius along the major axis of the ellipse defining the observed detection extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmjr_axis_raw_s1 sigma radius along the major axis of the ellipse defining the observed detection extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmjr_axis_raw_u1 sigma radius along the major axis of the ellipse defining the observed detection extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmjr_axis_raw_w1 sigma radius along the major axis of the ellipse defining the observed detection extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmjr_axis_raw_lolim_b1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmjr_axis_raw_lolim_h1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmjr_axis_raw_lolim_m1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmjr_axis_raw_lolim_s1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmjr_axis_raw_lolim_u1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmjr_axis_raw_lolim_w1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmjr_axis_raw_hilim_b1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmjr_axis_raw_hilim_h1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmjr_axis_raw_hilim_m1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmjr_axis_raw_hilim_s1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmjr_axis_raw_hilim_u1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmjr_axis_raw_hilim_w1 sigma radius along the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_b1 sigma radius along the minor axis of the ellipse defining the observed detection extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_h1 sigma radius along the minor axis of the ellipse defining the observed detection extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_m1 sigma radius along the minor axis of the ellipse defining the observed detection extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_s1 sigma radius along the minor axis of the ellipse defining the observed detection extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmnr_axis_raw_u1 sigma radius along the minor axis of the ellipse defining the observed detection extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmnr_axis_raw_w1 sigma radius along the minor axis of the ellipse defining the observed detection extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_lolim_b1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_lolim_h1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_lolim_m1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_lolim_s1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmnr_axis_raw_lolim_u1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmnr_axis_raw_lolim_w1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_hilim_b1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_hilim_h1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_hilim_m1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmnr_axis_raw_hilim_s1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmnr_axis_raw_hilim_u1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmnr_axis_raw_hilim_w1 sigma radius along the minor axis of the ellipse defining the observed detection extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpos_angle_raw_bPosition angle of the major axis of the ellipse defining the observed detection extent; ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_raw_hPosition angle of the major axis of the ellipse defining the observed detection extent; ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_raw_mPosition angle of the major axis of the ellipse defining the observed detection extent; ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_raw_sPosition angle of the major axis of the ellipse defining the observed detection extent; ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_raw_uPosition angle of the major axis of the ellipse defining the observed detection extent; ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_raw_wPosition angle of the major axis of the ellipse defining the observed detection extent; HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpos_angle_raw_lolim_bPosition angle of the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_raw_lolim_hPosition angle of the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_raw_lolim_mPosition angle of the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_raw_lolim_sPosition angle of the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_raw_lolim_uPosition angle of the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_raw_lolim_wPosition angle of the major axis of the ellipse defining the observed detection extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpos_angle_raw_hilim_bPosition angle of the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_raw_hilim_hPosition angle of the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_raw_hilim_mPosition angle of the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_raw_hilim_sPosition angle of the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_raw_hilim_uPosition angle of the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_raw_hilim_wPosition angle of the major axis of the ellipse defining the observed detection extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpsf_mjr_axis_raw_b1 sigma radius along the major axis of the ellipse defining the local PSF extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_h1 sigma radius along the major axis of the ellipse defining the local PSF extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_m1 sigma radius along the major axis of the ellipse defining the local PSF extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_s1 sigma radius along the major axis of the ellipse defining the local PSF extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_u1 sigma radius along the major axis of the ellipse defining the local PSF extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_w1 sigma radius along the major axis of the ellipse defining the local PSF extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_lolim_b1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_lolim_h1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_lolim_m1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_lolim_s1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_lolim_u1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_lolim_w1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_hilim_b1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_hilim_h1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_hilim_m1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_hilim_s1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_hilim_u1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEpsf_mjr_axis_raw_hilim_w1 sigma radius along the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_b1 sigma radius along the minor axis of the ellipse defining the local PSF extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_h1 sigma radius along the minor axis of the ellipse defining the local PSF extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_m1 sigma radius along the minor axis of the ellipse defining the local PSF extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_s1 sigma radius along the minor axis of the ellipse defining the local PSF extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_u1 sigma radius along the minor axis of the ellipse defining the local PSF extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_w1 sigma radius along the minor axis of the ellipse defining the local PSF extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_lolim_b1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_lolim_h1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_lolim_m1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_lolim_s1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_lolim_u1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_lolim_w1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_hilim_b1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_hilim_h1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_hilim_m1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_hilim_s1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_hilim_u1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEpsf_mnr_axis_raw_hilim_w1 sigma radius along the minor axis of the ellipse defining the local PSF extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpsf_pos_angle_raw_bPosition angle of the major axis of the ellipse defining the local PSF extent; ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpsf_pos_angle_raw_hPosition angle of the major axis of the ellipse defining the local PSF extent; ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpsf_pos_angle_raw_mPosition angle of the major axis of the ellipse defining the local PSF extent; ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpsf_pos_angle_raw_sPosition angle of the major axis of the ellipse defining the local PSF extent; ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpsf_pos_angle_raw_uPosition angle of the major axis of the ellipse defining the local PSF extent; ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpsf_pos_angle_raw_wPosition angle of the major axis of the ellipse defining the local PSF extent; HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpsf_pos_angle_raw_lolim_bPosition angle of the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpsf_pos_angle_raw_lolim_hPosition angle of the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpsf_pos_angle_raw_lolim_mPosition angle of the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpsf_pos_angle_raw_lolim_sPosition angle of the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpsf_pos_angle_raw_lolim_uPosition angle of the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpsf_pos_angle_raw_lolim_wPosition angle of the major axis of the ellipse defining the local PSF extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpsf_pos_angle_raw_hilim_bPosition angle of the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpsf_pos_angle_raw_hilim_hPosition angle of the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpsf_pos_angle_raw_hilim_mPosition angle of the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpsf_pos_angle_raw_hilim_sPosition angle of the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpsf_pos_angle_raw_hilim_uPosition angle of the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpsf_pos_angle_raw_hilim_wPosition angle of the major axis of the ellipse defining the local PSF extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEmajor_axis_b1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_h1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_m1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_s1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_u1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_w1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_b1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_h1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_m1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_lolim_s1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_lolim_u1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_lolim_w1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_b1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_h1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_m1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmajor_axis_hilim_s1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmajor_axis_hilim_u1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmajor_axis_hilim_w1 sigma radius along the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_b1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_h1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_m1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_s1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_u1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_w1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_b1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_h1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_m1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_lolim_s1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_lolim_u1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_lolim_w1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_b1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_h1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_m1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEminor_axis_hilim_s1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEminor_axis_hilim_u1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEminor_axis_hilim_w1 sigma radius along the minor axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpos_angle_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent; HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpos_angle_lolim_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_lolim_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_lolim_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_lolim_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_lolim_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_lolim_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEpos_angle_hilim_bPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_hilim_hPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_hilim_mPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_hilim_sPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_hilim_uPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_hilim_wPosition angle (ref. local true north) of the major axis of the ellipse defining the deconvolved detection extent (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banddegDOUBLEsrc_area_bArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; ACIS broad (0.5-7.0 keV) energy bandarcsec**2DOUBLEsrc_area_hArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; ACIS hard (2.0-7.0 keV) energy bandarcsec**2DOUBLEsrc_area_mArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; ACIS medium (1.2-2.0 keV) energy bandarcsec**2DOUBLEsrc_area_sArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; ACIS soft (0.5-1.2 keV) energy bandarcsec**2DOUBLEsrc_area_uArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsec**2DOUBLEsrc_area_wArea of the deconvolved detection extent ellipse, or area of the detection polygon for extended detections; HRC wide (~0.1-10.0 keV) energy bandarcsec**2DOUBLEphot_nsrcsNumber of detections fit simultaneously to compute aperture photometry quantitiesINTEGERcnts_aper_bTotal counts observed in the modified source region aperture; ACIS broad (0.5-7.0 keV) energy bandcountINTEGERcnts_aper_hTotal counts observed in the modified source region aperture; ACIS hard (2.0-7.0 keV) energy bandcountINTEGERcnts_aper_mTotal counts observed in the modified source region aperture; ACIS medium (1.2-2.0 keV) energy bandcountINTEGERcnts_aper_sTotal counts observed in the modified source region aperture; ACIS soft (0.5-1.2 keV) energy bandcountINTEGERcnts_aper_uTotal counts observed in the modified source region aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcountINTEGERcnts_aper_wTotal counts observed in the modified source region aperture; HRC wide (~0.1-10.0 keV) energy bandcountINTEGERcnts_aperbkg_bTotal counts observed in the modified background region aperture; ACIS broad (0.5-7.0 keV) energy bandcountINTEGERcnts_aperbkg_hTotal counts observed in the modified background region aperture; ACIS hard (2.0-7.0 keV) energy bandcountINTEGERcnts_aperbkg_mTotal counts observed in the modified background region aperture; ACIS medium (1.2-2.0 keV) energy bandcountINTEGERcnts_aperbkg_sTotal counts observed in the modified background region aperture; ACIS soft (0.5-1.2 keV) energy bandcountINTEGERcnts_aperbkg_uTotal counts observed in the modified background region aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcountINTEGERcnts_aperbkg_wTotal counts observed in the modified background region aperture; HRC wide (~0.1-10.0 keV) energy bandcountINTEGERcnts_aper90_bTotal counts observed in the modified PSF 90% ECF aperture; ACIS broad (0.5-7.0 keV) energy bandcountINTEGERcnts_aper90_hTotal counts observed in the modified PSF 90% ECF aperture; ACIS hard (2.0-7.0 keV) energy bandcountINTEGERcnts_aper90_mTotal counts observed in the modified PSF 90% ECF aperture; ACIS medium (1.2-2.0 keV) energy bandcountINTEGERcnts_aper90_sTotal counts observed in the modified PSF 90% ECF aperture; ACIS soft (0.5-1.2 keV) energy bandcountINTEGERcnts_aper90_uTotal counts observed in the modified PSF 90% ECF aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcountINTEGERcnts_aper90_wTotal counts observed in the modified PSF 90% ECF aperture; HRC wide (~0.1-10.0 keV) energy bandcountINTEGERcnts_aper90bkg_bTotal counts observed in the modified PSF 90% ECF background aperture; ACIS broad (0.5-7.0 keV) energy bandcountINTEGERcnts_aper90bkg_hTotal counts observed in the modified PSF 90% ECF background aperture; ACIS hard (2.0-7.0 keV) energy bandcountINTEGERcnts_aper90bkg_mTotal counts observed in the modified PSF 90% ECF background aperture; ACIS medium (1.2-2.0 keV) energy bandcountINTEGERcnts_aper90bkg_sTotal counts observed in the modified PSF 90% ECF background aperture; ACIS soft (0.5-1.2 keV) energy bandcountINTEGERcnts_aper90bkg_uTotal counts observed in the modified PSF 90% ECF background aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcountINTEGERcnts_aper90bkg_wTotal counts observed in the modified PSF 90% ECF background aperture; HRC wide (~0.1-10.0 keV) energy bandcountINTEGERsrc_cnts_aper_bAperture-corrected detection net counts inferred from the source region aperture; ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_hAperture-corrected detection net counts inferred from the source region aperture; ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_mAperture-corrected detection net counts inferred from the source region aperture; ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper_sAperture-corrected detection net counts inferred from the source region aperture; ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper_uAperture-corrected detection net counts inferred from the source region aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper_wAperture-corrected detection net counts inferred from the source region aperture; HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_bAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_hAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_mAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_sAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_uAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper_lolim_wAperture-corrected detection net counts inferred from the source region aperture (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_bAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_hAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_mAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_sAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_uAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper_hilim_wAperture-corrected detection net counts inferred from the source region aperture (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_bAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_hAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_mAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_sAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper90_uAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper90_wAperture-corrected detection net counts inferred from the PSF 90% ECF aperture; HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_bAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_hAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_mAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_sAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_uAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper90_lolim_wAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_bAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_hAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_mAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_sAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_uAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcountDOUBLEsrc_cnts_aper90_hilim_wAperture-corrected detection net counts inferred from the PSF 90% ECF aperture (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandcountDOUBLEra_aper90_bCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS right ascension; ACIS broad (0.5-7.0 keV) energy banddegpos.eq.ra;instr.fovDOUBLEra_aper90_hCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS right ascension; ACIS hard (2.0-7.0 keV) energy banddegpos.eq.ra;instr.fovDOUBLEra_aper90_mCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS right ascension; ACIS medium (1.2-2.0 keV) energy banddegpos.eq.ra;instr.fovDOUBLEra_aper90_sCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS right ascension; ACIS soft (0.5-1.2 keV) energy banddegpos.eq.ra;instr.fovDOUBLEra_aper90_uCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS right ascension; ACIS ultrasoft (0.2-0.5 keV) energy banddegpos.eq.ra;instr.fovDOUBLEra_aper90_wCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS right ascension; HRC wide (~0.1-10.0 keV) energy banddegpos.eq.ra;instr.fovDOUBLEdec_aper90_bCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS declination; ACIS broad (0.5-7.0 keV) energy banddegpos.eq.dec;instr.fovDOUBLEdec_aper90_hCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS declination; ACIS hard (2.0-7.0 keV) energy banddegpos.eq.dec;instr.fovDOUBLEdec_aper90_mCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS declination; ACIS medium (1.2-2.0 keV) energy banddegpos.eq.dec;instr.fovDOUBLEdec_aper90_sCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS declination; ACIS soft (0.5-1.2 keV) energy banddegpos.eq.dec;instr.fovDOUBLEdec_aper90_uCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS declination; ACIS ultrasoft (0.2-0.5 keV) energy banddegpos.eq.dec;instr.fovDOUBLEdec_aper90_wCenter of the PSF 90% ECF and PSF 90% ECF background apertures, ICRS declination; HRC wide (~0.1-10.0 keV) energy banddegpos.eq.dec;instr.fovDOUBLEmjr_axis_aper90_bSemi-major axis of the elliptical PSF 90% ECF aperture; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmjr_axis_aper90_hSemi-major axis of the elliptical PSF 90% ECF aperture; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmjr_axis_aper90_mSemi-major axis of the elliptical PSF 90% ECF aperture; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmjr_axis_aper90_sSemi-major axis of the elliptical PSF 90% ECF aperture; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmjr_axis_aper90_uSemi-major axis of the elliptical PSF 90% ECF aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmjr_axis_aper90_wSemi-major axis of the elliptical PSF 90% ECF aperture; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmnr_axis_aper90_bSemi-minor axis of the elliptical PSF 90% ECF aperture; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmnr_axis_aper90_hSemi-minor axis of the elliptical PSF 90% ECF aperture; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmnr_axis_aper90_mSemi-minor axis of the elliptical PSF 90% ECF aperture; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmnr_axis_aper90_sSemi-minor axis of the elliptical PSF 90% ECF aperture; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmnr_axis_aper90_uSemi-minor axis of the elliptical PSF 90% ECF aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmnr_axis_aper90_wSemi-minor axis of the elliptical PSF 90% ECF aperture; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpos_angle_aper90_bPosition angle (ref. local true north) of the semi-major axis of the elliptical PSF 90% ECF aperture; ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_aper90_hPosition angle (ref. local true north) of the semi-major axis of the elliptical PSF 90% ECF aperture; ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_aper90_mPosition angle (ref. local true north) of the semi-major axis of the elliptical PSF 90% ECF aperture; ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_aper90_sPosition angle (ref. local true north) of the semi-major axis of the elliptical PSF 90% ECF aperture; ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_aper90_uPosition angle (ref. local true north) of the semi-major axis of the elliptical PSF 90% ECF aperture; ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_aper90_wPosition angle (ref. local true north) of the semi-major axis of the elliptical PSF 90% ECF aperture; HRC wide (~0.1-10.0 keV) energy banddegDOUBLEmjr_axis1_aper90bkg_bSemi-major axis of the inner ellipse of the annular PSF 90% ECF background aperture; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmjr_axis1_aper90bkg_hSemi-major axis of the inner ellipse of the annular PSF 90% ECF background aperture; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmjr_axis1_aper90bkg_mSemi-major axis of the inner ellipse of the annular PSF 90% ECF background aperture; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmjr_axis1_aper90bkg_sSemi-major axis of the inner ellipse of the annular PSF 90% ECF background aperture; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmjr_axis1_aper90bkg_uSemi-major axis of the inner ellipse of the annular PSF 90% ECF background aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmjr_axis1_aper90bkg_wSemi-major axis of the inner ellipse of the annular PSF 90% ECF background aperture; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmnr_axis1_aper90bkg_bSemi-minor axis of the inner ellipse of the annular PSF 90% ECF background aperture; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmnr_axis1_aper90bkg_hSemi-minor axis of the inner ellipse of the annular PSF 90% ECF background aperture; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmnr_axis1_aper90bkg_mSemi-minor axis of the inner ellipse of the annular PSF 90% ECF background aperture; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmnr_axis1_aper90bkg_sSemi-minor axis of the inner ellipse of the annular PSF 90% ECF background aperture; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmnr_axis1_aper90bkg_uSemi-minor axis of the inner ellipse of the annular PSF 90% ECF background aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmnr_axis1_aper90bkg_wSemi-minor axis of the inner ellipse of the annular PSF 90% ECF background aperture; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmjr_axis2_aper90bkg_bSemi-major axis of the outer ellipse of the annular PSF 90% ECF background aperture; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmjr_axis2_aper90bkg_hSemi-major axis of the outer ellipse of the annular PSF 90% ECF background aperture; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmjr_axis2_aper90bkg_mSemi-major axis of the outer ellipse of the annular PSF 90% ECF background aperture; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmjr_axis2_aper90bkg_sSemi-major axis of the outer ellipse of the annular PSF 90% ECF background aperture; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmjr_axis2_aper90bkg_uSemi-major axis of the outer ellipse of the annular PSF 90% ECF background aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmjr_axis2_aper90bkg_wSemi-major axis of the outer ellipse of the annular PSF 90% ECF background aperture; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEmnr_axis2_aper90bkg_bSemi-minor axis of the outer ellipse of the annular PSF 90% ECF background aperture; ACIS broad (0.5-7.0 keV) energy bandarcsecDOUBLEmnr_axis2_aper90bkg_hSemi-minor axis of the outer ellipse of the annular PSF 90% ECF background aperture; ACIS hard (2.0-7.0 keV) energy bandarcsecDOUBLEmnr_axis2_aper90bkg_mSemi-minor axis of the outer ellipse of the annular PSF 90% ECF background aperture; ACIS medium (1.2-2.0 keV) energy bandarcsecDOUBLEmnr_axis2_aper90bkg_sSemi-minor axis of the outer ellipse of the annular PSF 90% ECF background aperture; ACIS soft (0.5-1.2 keV) energy bandarcsecDOUBLEmnr_axis2_aper90bkg_uSemi-minor axis of the outer ellipse of the annular PSF 90% ECF background aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandarcsecDOUBLEmnr_axis2_aper90bkg_wSemi-minor axis of the outer ellipse of the annular PSF 90% ECF background aperture; HRC wide (~0.1-10.0 keV) energy bandarcsecDOUBLEpos_angle_aper90bkg_bPosition angle (ref. local true north) of the semi-major axes of the annular PSF 90% ECF background aperture; ACIS broad (0.5-7.0 keV) energy banddegDOUBLEpos_angle_aper90bkg_hPosition angle (ref. local true north) of the semi-major axes of the annular PSF 90% ECF background aperture; ACIS hard (2.0-7.0 keV) energy banddegDOUBLEpos_angle_aper90bkg_mPosition angle (ref. local true north) of the semi-major axes of the annular PSF 90% ECF background aperture; ACIS medium (1.2-2.0 keV) energy banddegDOUBLEpos_angle_aper90bkg_sPosition angle (ref. local true north) of the semi-major axes of the annular PSF 90% ECF background aperture; ACIS soft (0.5-1.2 keV) energy banddegDOUBLEpos_angle_aper90bkg_uPosition angle (ref. local true north) of the semi-major axes of the annular PSF 90% ECF background aperture; ACIS ultrasoft (0.2-0.5 keV) energy banddegDOUBLEpos_angle_aper90bkg_wPosition angle (ref. local true north) of the semi-major axes of the annular PSF 90% ECF background aperture; HRC wide (~0.1-10.0 keV) energy banddegDOUBLEarea_aper90_bArea of the modified elliptical PSF 90% ECF aperture (includes corrections for exclusion regions due to overlapping detections); ACIS broad (0.5-7.0 keV) energy bandarcsec**2DOUBLEarea_aper90_hArea of the modified elliptical PSF 90% ECF aperture (includes corrections for exclusion regions due to overlapping detections); ACIS hard (2.0-7.0 keV) energy bandarcsec**2DOUBLEarea_aper90_mArea of the modified elliptical PSF 90% ECF aperture (includes corrections for exclusion regions due to overlapping detections); ACIS medium (1.2-2.0 keV) energy bandarcsec**2DOUBLEarea_aper90_sArea of the modified elliptical PSF 90% ECF aperture (includes corrections for exclusion regions due to overlapping detections); ACIS soft (0.5-1.2 keV) energy bandarcsec**2DOUBLEarea_aper90_uArea of the modified elliptical PSF 90% ECF aperture (includes corrections for exclusion regions due to overlapping detections); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsec**2DOUBLEarea_aper90_wArea of the modified elliptical PSF 90% ECF aperture (includes corrections for exclusion regions due to overlapping detections); HRC wide (~0.1-10.0 keV) energy bandarcsec**2DOUBLEarea_aper90bkg_bArea of the modified annular PSF 90% ECF background aperture (includes corrections for exclusion regions due to overlapping detections); ACIS broad (0.5-7.0 keV) energy bandarcsec**2DOUBLEarea_aper90bkg_hArea of the modified annular PSF 90% ECF background aperture (includes corrections for exclusion regions due to overlapping detections); ACIS hard (2.0-7.0 keV) energy bandarcsec**2DOUBLEarea_aper90bkg_mArea of the modified annular PSF 90% ECF background aperture (includes corrections for exclusion regions due to overlapping detections); ACIS medium (1.2-2.0 keV) energy bandarcsec**2DOUBLEarea_aper90bkg_sArea of the modified annular PSF 90% ECF background aperture (includes corrections for exclusion regions due to overlapping detections); ACIS soft (0.5-1.2 keV) energy bandarcsec**2DOUBLEarea_aper90bkg_uArea of the modified annular PSF 90% ECF background aperture (includes corrections for exclusion regions due to overlapping detections); ACIS ultrasoft (0.2-0.5 keV) energy bandarcsec**2DOUBLEarea_aper90bkg_wArea of the modified annular PSF 90% ECF background aperture (includes corrections for exclusion regions due to overlapping detections); HRC wide (~0.1-10.0 keV) energy bandarcsec**2DOUBLEsrc_rate_aper_bAperture-corrected detection net count rate inferred from the source region aperture; ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_hAperture-corrected detection net count rate inferred from the source region aperture; ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_mAperture-corrected detection net count rate inferred from the source region aperture; ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_sAperture-corrected detection net count rate inferred from the source region aperture; ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper_uAperture-corrected detection net count rate inferred from the source region aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper_wAperture-corrected detection net count rate inferred from the source region aperture; HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_bAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_hAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_mAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_sAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_uAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper_lolim_wAperture-corrected detection net count rate inferred from the source region aperture (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_bAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_hAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_mAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_sAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_uAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper_hilim_wAperture-corrected detection net count rate inferred from the source region aperture (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_bAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_mAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_sAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper90_uAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper90_wAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture; HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_bAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_hAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_mAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_sAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_uAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper90_lolim_wAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_bAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_hAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_mAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_sAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_uAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEsrc_rate_aper90_hilim_wAperture-corrected detection net count rate inferred from the PSF 90% ECF aperture (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEphotflux_aper_bAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_mAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_sAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_uAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_wAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_bAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_hAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_mAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_sAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_uAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_lolim_wAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_bAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_hAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_mAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_sAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_uAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper_hilim_wAperture-corrected detection net photon flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_bAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_mAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_sAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_uAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_wAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_bAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_hAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_mAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_sAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_uAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_lolim_wAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_bAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_hAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_mAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_sAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_uAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy bandphoton/s/cm**2DOUBLEphotflux_aper90_hilim_wAperture-corrected detection net photon flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy bandphoton/s/cm**2DOUBLEflux_aper_bAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper_hAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_mAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_sAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_uAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_wAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper_lolim_bAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper_lolim_hAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_lolim_mAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_lolim_sAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_lolim_uAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_lolim_wAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper_hilim_bAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper_hilim_hAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_hilim_mAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper_hilim_sAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper_hilim_uAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper_hilim_wAperture-corrected detection net energy flux inferred from the source region aperture, calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEprincipalflux_aper90_bAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_mAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_sAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_uAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_wAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_bAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_hAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_mAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_sAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_uAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_lolim_wAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_bAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_hAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_mAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_sAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_uAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_aper90_hilim_wAperture-corrected detection net energy flux inferred from the PSF 90% ECF aperture, calculated by counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_bSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_mSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_sSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_uSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_wSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_powlaw_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed power law model [N_H = N_H(Gal); Gamma = 2.0] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_bSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_mSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_sSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_uSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_wSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_bb_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed black body model [N_H = N_H(Gal); kT = 0.75 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_bSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_mSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_sSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_uSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_wSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_brems_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed bremsstrahlung model [N_H = N_H(Gal); kT = 3.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_bSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_mSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_sSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_uSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_wSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_bSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_hSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_mSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_sSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_uSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_lolim_wSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_bSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_hSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_mSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_sSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_uSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper_hilim_wSource region aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV]; HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_lolim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_bPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_hPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_mPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_sPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_uPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy banderg/s/cm**2DOUBLEflux_apec_aper90_hilim_wPSF 90% ECF aperture model energy flux inferred from the canonical absorbed APEC model [N_H = N_H(Gal); kT = 6.5 keV] (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy banderg/s/cm**2DOUBLEpsf_frac_aper_bFraction of the PSF included in the modified elliptical source region aperture; ACIS broad (0.5-7.0 keV) energy bandDOUBLEpsf_frac_aper_hFraction of the PSF included in the modified elliptical source region aperture; ACIS hard (2.0-7.0 keV) energy bandDOUBLEpsf_frac_aper_mFraction of the PSF included in the modified elliptical source region aperture; ACIS medium (1.2-2.0 keV) energy bandDOUBLEpsf_frac_aper_sFraction of the PSF included in the modified elliptical source region aperture; ACIS soft (0.5-1.2 keV) energy bandDOUBLEpsf_frac_aper_uFraction of the PSF included in the modified elliptical source region aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEpsf_frac_aper_wFraction of the PSF included in the modified elliptical source region aperture; HRC wide (~0.1-10.0 keV) energy bandDOUBLEpsf_frac_aperbkg_bFraction of the PSF included in the modified annular background region aperture; ACIS broad (0.5-7.0 keV) energy bandDOUBLEpsf_frac_aperbkg_hFraction of the PSF included in the modified annular background region aperture; ACIS hard (2.0-7.0 keV) energy bandDOUBLEpsf_frac_aperbkg_mFraction of the PSF included in the modified annular background region aperture; ACIS medium (1.2-2.0 keV) energy bandDOUBLEpsf_frac_aperbkg_sFraction of the PSF included in the modified annular background region aperture; ACIS soft (0.5-1.2 keV) energy bandDOUBLEpsf_frac_aperbkg_uFraction of the PSF included in the modified annular background region aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEpsf_frac_aperbkg_wFraction of the PSF included in the modified annular background region aperture; HRC wide (~0.1-10.0 keV) energy bandDOUBLEpsf_frac_aper90_bFraction of the PSF included in the modified elliptical PSF 90% ECF aperture; ACIS broad (0.5-7.0 keV) energy bandDOUBLEpsf_frac_aper90_hFraction of the PSF included in the modified elliptical PSF 90% ECF aperture; ACIS hard (2.0-7.0 keV) energy bandDOUBLEpsf_frac_aper90_mFraction of the PSF included in the modified elliptical PSF 90% ECF aperture; ACIS medium (1.2-2.0 keV) energy bandDOUBLEpsf_frac_aper90_sFraction of the PSF included in the modified elliptical PSF 90% ECF aperture; ACIS soft (0.5-1.2 keV) energy bandDOUBLEpsf_frac_aper90_uFraction of the PSF included in the modified elliptical PSF 90% ECF aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEpsf_frac_aper90_wFraction of the PSF included in the modified elliptical PSF 90% ECF aperture; HRC wide (~0.1-10.0 keV) energy bandDOUBLEpsf_frac_aper90bkg_bFraction of the PSF included in the modified annular PSF 90% ECF background aperture; ACIS broad (0.5-7.0 keV) energy bandDOUBLEpsf_frac_aper90bkg_hFraction of the PSF included in the modified annular PSF 90% ECF background aperture; ACIS hard (2.0-7.0 keV) energy bandDOUBLEpsf_frac_aper90bkg_mFraction of the PSF included in the modified annular PSF 90% ECF background aperture; ACIS medium (1.2-2.0 keV) energy bandDOUBLEpsf_frac_aper90bkg_sFraction of the PSF included in the modified annular PSF 90% ECF background aperture; ACIS soft (0.5-1.2 keV) energy bandDOUBLEpsf_frac_aper90bkg_uFraction of the PSF included in the modified annular PSF 90% ECF background aperture; ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEpsf_frac_aper90bkg_wFraction of the PSF included in the modified annular PSF 90% ECF background aperture; HRC wide (~0.1-10.0 keV) energy bandDOUBLEflux_powlawNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_powlaw_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_powlaw_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEpowlaw_gammaPhoton index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_gamma_lolimPhoton index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEpowlaw_gamma_hilimPhoton index, defined as F_E ~ E^(-Gamma), of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)DOUBLEpowlaw_gamma_rhatPhoton index convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_nhN_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEpowlaw_nh_lolimN_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEpowlaw_nh_hilimN_H column density of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEpowlaw_nh_rhatN_H column density convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_amplAmplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_ampl_lolimAmplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEpowlaw_ampl_hilimAmplitude of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEpowlaw_ampl_rhatAmplitude convergence criterion of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEpowlaw_statchi-square statistic per degree of freedom of the best fitting absorbed power-law model spectrum to the source region aperture PI spectrumDOUBLEflux_bbNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_bb_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_bb_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEbb_ktTemperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumkeVDOUBLEbb_kt_lolimTemperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)keVDOUBLEbb_kt_hilimTemperature (kT) of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)keVDOUBLEbb_kt_rhatTemperature (kT) convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_nhN_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEbb_nh_lolimN_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEbb_nh_hilimN_H column density of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEbb_nh_rhatN_H column density convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_amplAmplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_ampl_lolimAmplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEbb_ampl_hilimAmplitude of the best fitting absorbed black body model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEbb_ampl_rhatAmplitude convergence criterion of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEbb_statchi-square statistic per degree of freedom of the best fitting absorbed black body model spectrum to the source region aperture PI spectrumDOUBLEflux_bremsNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_brems_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_brems_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEbrems_ktTemperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumkeVDOUBLEbrems_kt_lolimTemperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)keVDOUBLEbrems_kt_hilimTemperature (kT) of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)keVDOUBLEbrems_kt_rhatTemperature (kT) convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_nhN_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEbrems_nh_lolimN_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEbrems_nh_hilimN_H column density of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEbrems_nh_rhatN_H column density convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_normAmplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_norm_lolimAmplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEbrems_norm_hilimAmplitude of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEbrems_norm_rhatAmplitude convergence criterion of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEbrems_statchi-square statistic per degree of freedom of the best fitting absorbed bremsstrahlung model spectrum to the source region aperture PI spectrumDOUBLEflux_apecNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumerg/s/cm**2DOUBLEflux_apec_lolimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)erg/s/cm**2DOUBLEflux_apec_hilimNet integrated 0.5-7.0 keV energy flux of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)erg/s/cm**2DOUBLEapec_ktTemperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumkeVDOUBLEapec_kt_lolimTemperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)keVDOUBLEapec_kt_hilimTemperature (kT) of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)keVDOUBLEapec_kt_rhatTemperature (kT) convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_abundAbundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_abund_lolimAbundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEapec_abund_hilimAbundance of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)DOUBLEapec_abund_rhatAbundance convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_zRedshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_z_lolimRedshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEapec_z_hilimRedshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)DOUBLEapec_z_rhatRedshift convergence criterion Redshift of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_nhN_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum10**20/cm**2DOUBLEapec_nh_lolimN_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)10**20/cm**2DOUBLEapec_nh_hilimN_H column density of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upper confidence limit)10**20/cm**2DOUBLEapec_nh_rhatN_H column density convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_normAmplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_norm_lolimAmplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% lower confidence limit)DOUBLEapec_norm_hilimAmplitude of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrum (68% upperer confidence limit)DOUBLEapec_norm_rhatAmplitude convergence criterion of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEapec_statchi-square statistic per degree of freedom of the best fitting absorbed APEC model spectrum to the source region aperture PI spectrumDOUBLEhard_hmACIS hard - medium (1.2-2.0 keV) energy band hardness ratioDOUBLEhard_hm_lolimACIS hard - medium (1.2-2.0 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_hm_hilimACIS hard - medium (1.2-2.0 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEhard_hsACIS hard - soft (0.5-1.2 keV) energy band hardness ratioDOUBLEhard_hs_lolimACIS hard - soft (0.5-1.2 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_hs_hilimACIS hard - soft (0.5-1.2 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEhard_msACIS medium - soft (0.5-1.2 keV) energy band hardness ratioDOUBLEhard_ms_lolimACIS medium - soft (0.5-1.2 keV) energy band hardness ratio (68% lower confidence limit)DOUBLEhard_ms_hilimACIS medium - soft (0.5-1.2 keV) energy band hardness ratio (68% upper confidence limit)DOUBLEks_prob_bIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEks_prob_hIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEks_prob_mIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEks_prob_sIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEks_prob_uIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEks_prob_wIntra-observation Kolmogorov-Smirnov test variability probability (highest value across all observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEkp_prob_bIntra-observation Kuiper's test variability probability (highest value across all stacked observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEkp_prob_hIntra-observation Kuiper's test variability probability (highest value across all stacked observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEkp_prob_mIntra-observation Kuiper's test variability probability (highest value across all stacked observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEkp_prob_sIntra-observation Kuiper's test variability probability (highest value across all stacked observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEkp_prob_uIntra-observation Kuiper's test variability probability (highest value across all stacked observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEkp_prob_wIntra-observation Kuiper's test variability probability (highest value across all stacked observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEvar_prob_bIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); ACIS broad (0.5-7.0 keV) energy bandDOUBLEvar_prob_hIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); ACIS hard (2.0-7.0 keV) energy bandDOUBLEvar_prob_mIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); ACIS medium (1.2-2.0 keV) energy bandDOUBLEvar_prob_sIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); ACIS soft (0.5-1.2 keV) energy bandDOUBLEvar_prob_uIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); ACIS ultrasoft (0.2-0.5 keV) energy bandDOUBLEvar_prob_wIntra-observation Gregory-Loredo variability probability (highest value across all stacked observations); HRC wide (~0.1-10.0 keV) energy bandDOUBLEvar_index_bIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); ACIS broad (0.5-7.0 keV) energy bandINTEGERvar_index_hIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); ACIS hard (2.0-7.0 keV) energy bandINTEGERvar_index_mIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); ACIS medium (1.2-2.0 keV) energy bandINTEGERvar_index_sIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); ACIS soft (0.5-1.2 keV) energy bandINTEGERvar_index_uIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); ACIS ultrasoft (0.2-0.5 keV) energy bandINTEGERvar_index_wIntra-observation Gregory-Loredo variability index in the range [0, 10]: indicates whether the source region photon flux is constant within an observation (highest value across all stacked observations); HRC wide (~0.1-10.0 keV) energy bandINTEGERvar_mean_bFlux variability mean value, calculated from an optimally-binned light curve; ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEvar_mean_hFlux variability mean value, calculated from an optimally-binned light curve; ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEvar_mean_mFlux variability mean value, calculated from an optimally-binned light curve; ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEvar_mean_sFlux variability mean value, calculated from an optimally-binned light curve; ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEvar_mean_uFlux variability mean value, calculated from an optimally-binned light curve; ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEvar_mean_wFlux variability mean value, calculated from an optimally-binned light curve; HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEvar_sigma_bFlux variability standard deviation, calculated from an optimally-binned light curve; ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEvar_sigma_hFlux variability standard deviation, calculated from an optimally-binned light curve; ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEvar_sigma_mFlux variability standard deviation, calculated from an optimally-binned light curve; ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEvar_sigma_sFlux variability standard deviation, calculated from an optimally-binned light curve; ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEvar_sigma_uFlux variability standard deviation, calculated from an optimally-binned light curve; ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEvar_sigma_wFlux variability standard deviation, calculated from an optimally-binned light curve; HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEvar_min_bFlux variability minimum value, calculated from an optimally-binned light curve; ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEvar_min_hFlux variability minimum value, calculated from an optimally-binned light curve; ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEvar_min_mFlux variability minimum value, calculated from an optimally-binned light curve; ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEvar_min_sFlux variability minimum value, calculated from an optimally-binned light curve; ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEvar_min_uFlux variability minimum value, calculated from an optimally-binned light curve; ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEvar_min_wFlux variability minimum value, calculated from an optimally-binned light curve; HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEvar_max_bFlux variability maximum value, calculated from an optimally-binned light curve; ACIS broad (0.5-7.0 keV) energy bandcount/sDOUBLEvar_max_hFlux variability maximum value, calculated from an optimally-binned light curve; ACIS hard (2.0-7.0 keV) energy bandcount/sDOUBLEvar_max_mFlux variability maximum value, calculated from an optimally-binned light curve; ACIS medium (1.2-2.0 keV) energy bandcount/sDOUBLEvar_max_sFlux variability maximum value, calculated from an optimally-binned light curve; ACIS soft (0.5-1.2 keV) energy bandcount/sDOUBLEvar_max_uFlux variability maximum value, calculated from an optimally-binned light curve; ACIS ultrasoft (0.2-0.5 keV) energy bandcount/sDOUBLEvar_max_wFlux variability maximum value, calculated from an optimally-binned light curve; HRC wide (~0.1-10.0 keV) energy bandcount/sDOUBLEdither_warning_flagHighest statistically significant peak in the power spectrum of the detection source region count rate occurs at the dither frequency or at a beat frequency of the dither frequency of the observationBOOLEANlivetimeEffective single observation exposure time at the location of the detection, after applying the good time intervals and the deadtime correction factorsDOUBLEprincipaldetectorDetector elements over which the background region bounding box dithers during the observationVARCHARcsc21.master_stack_assocMaster Source/Stack Source AssociationsnameMaster Source identifiermeta.idVARCHARprincipaldetect_stack_idStack Source identifiermeta.idVARCHARregion_idStack Source identifiermeta.idINTEGERprincipalmatch_typeType of matchmeta.codeVARCHARcsc21.master_sourcenamenamecsc21.stack_sourcedetect_stack_iddetect_stack_idregion_idregion_idcsc21.stack_observation_assocStack Source/Observation Source Associationsdetect_stack_idStack Source identifiermeta.idVARCHARobsidObservation identifiermeta.id;obs.paramINTEGERprincipalobiObservation interval numbermeta.id;obs.paramINTEGERprincipalcycleACIS readout cycle for the observation, 'P' (primary) or 'S' (secondary) for alternating exposure (interleaved) mode observations, or 'P' for other ACIS modesinstr.setupVARCHARregion_idStack Source identifiermeta.idINTEGERprincipalcsc21.stack_sourcedetect_stack_iddetect_stack_idregion_idregion_idcsc21.observation_sourceobsidobsidobiobiregion_idregion_idcsc21.detect_stackDetect Stack/Observation Associationsdetect_stack_idDetect stack identifiermeta.idVARCHARobsidObservation identifiermeta.id;obs.paramINTEGERprincipalobiObservation interval numbermeta.id;obs.paramINTEGERprincipalcycleACIS readout cycle for the observation, 'P' (primary) or 'S' (secondary) for alternating exposure (interleaved) mode observations, or 'P' for other ACIS modesinstr.setupVARCHARcsc21.stack_sourcedetect_stack_iddetect_stack_idcsc21.observation_sourceobsidobsidobiobicsc21.valid_stackValid Stack/Per-Observation Detection Associationsdetect_stack_idStack Source identifiermeta.idVARCHARregion_idDetect region identifiermeta.idINTEGERprincipalobsidObservation identifiermeta.id;obs.paramINTEGERprincipalobiObservation interval numbermeta.id;obs.paramINTEGERprincipalcycleACIS readout cycle for the observation, 'P' (primary) or 'S' (secondary) for alternating exposure (interleaved) mode observations, or 'P' for other ACIS modesinstr.setupVARCHARcsc21.stack_sourcedetect_stack_iddetect_stack_idregion_idregion_idcsc21.observation_sourceobsidobsidobiobiregion_idregion_idcsc21.likely_stackLikely Stack/Per-Observation Detection Associationsdetect_stack_idDetect stack identifiermeta.idVARCHARregion_idDetect region identifiermeta.idINTEGERprincipalobsidObservation identifiermeta.id;obs.paramINTEGERprincipalobiObservation interval numbermeta.id;obs.paramINTEGERprincipalcycleACIS readout cycle for the observation, 'P' (primary) or 'S' (secondary) for alternating exposure (interleaved) mode observations, or 'P' for other ACIS modesinstr.setupVARCHARcsc21.stack_sourcedetect_stack_iddetect_stack_idregion_idregion_idcsc21.observation_sourceobsidobsidobiobiregion_idregion_idcsc21.imageSIAP images viewcoordrefWCS Coordinate PixelVOX:WCS_CoordPixelDOUBLEprincipalcdmatrixWCS CD MatrixVOX:WCS_CDMatrixDOUBLEprincipalbandBandVOX:BandPass_IDVARCHARprincipalbandrefBand Reference ValueVOX:BandPass_RefValueDOUBLEprincipalbandloBand LoVOX:BandPass_LoLimitDOUBLEprincipalbandhiBand HiVOX:BandPass_HiLimitDOUBLEprincipalnameTitleVOX:Image_TitleVARCHARprincipalinstrumentInstrumentVOX:INST_IDVARCHARprincipaldate_obsEpoch at midpoint of observationdVOX:Image_MJDateObsDOUBLEprincipalraSource position, ICRS right ascensiondegPOS_EQ_RA_MAINstc:AstroCoords.Position2D.Value2.C1DOUBLEprincipaldecSource position, ICRS declinationdegPOS_EQ_DEC_MAINstc:AstroCoords.Position2D.Value2.C2DOUBLEprincipalnaxisArray of length in pixels of each image axisVOX:Image_NaxisINTEGERprincipalimgscaleArray of image scale for each image axisdeg/pixelVOX:Image_ScaleDOUBLEprincipalimgfmtMIME-type of the object associated with the image access referenceVOX:Image_FormatVARCHARprincipalpixflagsFlags specifying processing of image (C:copy without change)VOX:Image_PixFlagsVARCHARprincipalaccrefAccess referenceVOX:Image_AccessReferenceVARCHARprincipalfilesizeFilesizebyteVOX:Image_FileSizeINTEGERprincipalgti_elapseTotal elapsed time of the observation (gti_stop - gti_start)sDOUBLEivoaInternational Virtual Observatory Allianceivoa.ObsCoreObsCore 1.0dataproduct_typeLogical data product typemeta.code.classobscore:ObsDataset.dataProductTypeVARCHARcalib_levelCalibration levelmeta.code;obs.calibobscore:ObsDataset.calibLevelINTEGERobs_collectionName of the data collectionmeta.idobscore:DataID.CollectionVARCHARobs_idStack detect IDmeta.idobscore:DataID.observationIDVARCHARobs_publisher_didDataset identifier given by the publishermeta.ref.ivoidobscore:Curation.PublisherDIDVARCHARaccess_formatFile content formatmeta.code.mimeobscore:Access.FormatVARCHARs_raCentral right ascension, ICRSdegpos.eq.raobscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C1DOUBLEs_decCentral declination, ICRSdegpos.eq.decobscore:Char.SpatialAxis.Coverage.Location.Coord.Position2D.Value2.C2DOUBLEs_fovDiameter (bounds) of the covered regiondegphys.angSize;instr.fovobscore:Char.SpatialAxis.Coverage.Bounds.Extent.diameterDOUBLEs_regionRegion covered as specified in STC or ADQLpos.outline;obs.fieldobscore:Char.SpatialAxis.Coverage.Support.AreaREGIONs_resolutionSpatial resolution of data as FWHMarcsecpos.angResolutionobscore:Char.SpatialAxis.Resolution.Refval.valueDOUBLEt_exptimeTotal exposure timestime.duration;obs.exposureobscore:Char.TimeAxis.Coverage.Support.ExtentDOUBLEem_minStart in spectral coordinatesmem.wl;stat.minobscore:Char.SpectralAxis.Coverage.Bounds.Limits.LoLimitDOUBLEem_maxStop in spectral coordinatesmem.wl;stat.maxobscore:Char.SpectralAxis.Coverage.Bounds.Limits.HiLimitDOUBLEo_ucdUCD of observable (e.g. phot.flux.density)meta.ucdobscore:Char.ObservableAxis.ucdVARCHARpol_statesList of polarization states or NULL if not applicablemeta.code;phys.polarizationobscore:Char.PolarizationAxis.stateListVARCHARfacility_nameFacilitymeta.id;instr.telobscore:Provenance.ObsConfig.Facility.nameVARCHARinstrument_nameName of the instrument used for this stackmeta.id;instrobscore:Provenance.ObsConfig.Instrument.nameVARCHARobs_creation_dateDate when the dataset was createdtime;meta.datasetobscore:DataID.DateTIMESTAMPobs_creator_nameName of the creator of the datameta.idobscore:DataID.CreatorVARCHARobs_creator_didIVOA dataset identifier given by the creatormeta.idobscore:DataID.CreatorDIDVARCHARobs_titleBrief description of dataset in free formatmeta.title;obsobscore:DataID.TitleVARCHARpublisher_idIVOA-ID for the Publishermeta.ref.ivoidobscore:Curation.PublisherIDVARCHARdata_rightsData rightsmeta.codeobscore:Curation.RightsVARCHARobs_release_dateDate of final release of associated CSC versiontime.releaseobscore:Curation.releaseDateTIMESTAMPs_resolution_minResolution min value on spectral axis (FHWM of PSF)arcsecpos.angResolution;stat.minobscore:Char.SpatialAxis.Resolution.Bounds.Limits.LoLimitDOUBLEs_resolution_maxResolution max value on spectral axisarcsecpos.angResolution;stat.maxobscore:Char.SpatialAxis.Resolution.Bounds.Limits.HiLimitDOUBLEs_calib_statusType of calibration along the spatial axismeta.code.qualobscore:Char.SpatialAxis.calibrationStatusVARCHARs_stat_errorAstrometric precision along the spatial axisarcsecstat.error;pos.eqobscore:Char.SpatialAxis.Accuracy.statError.refval.valueDOUBLEt_calib_statusType of time coord calibrationmeta.code.qualobscore:Char.TimeAxis.calibrationStatusVARCHARem_ucdNature of the spectral axismeta.ucdobscore:Char.SpectralAxis.ucdVARCHARem_unitUnits along the spectral axismeta.unitobscore:Char.SpectralAxis.unitVARCHARem_res_power_minResolving power min value on spectral axisspect.resolution;stat.minobscore:Char.SpectralAxis.Resolution.ResolPower.LoLimitDOUBLEem_res_power_maxResolving power max value on spectral axisspect.resolution;stat.maxobscore:Char.SpectralAxis.Resolution.ResolPower.HiLimitDOUBLEem_calib_statusType of spectral coord calibrationmeta.code.qualobscore:Char.SpectralAxis.calibrationStatusVARCHARo_unitUnits used for the observable valuesmeta.unitobscore:Char.ObservableAxis.unitVARCHARo_calib_statusLevel of calibration for the observable coordmeta.code.qualobscore:Char.ObservableAxis.calibrationStatusVARCHARo_stat_error_typeErrorstat.errorVARCHARaccrefAccess referenceVOX:Image_AccessReferenceVARCHARaccess_urlURL used to access (download) datasetmeta.ref.urlobscore:Access.ReferenceCLOBaccess_estsizeEstimated size of dataset in kBkbytephys.size;meta.fileobscore:Access.SizeBIGINTt_minStart time in MJDdtime.start;obs.exposureobscore:Char.TimeAxis.Coverage.Bounds.Limits.StartTimeDOUBLEt_maxStop time in MJDdtime.end;obs.exposureobscore:Char.TimeAxis.Coverage.Bounds.Limits.StopTimeDOUBLEt_resolutionTemporal resolution FWHMstime.resolutionobscore:Char.TimeAxis.Resolution.Refval.valueDOUBLEem_res_powerSpectral resolving powerspect.resolutionobscore:Char.SpectralAxis.Resolution.resolpower.refvalDOUBLEdataproduct_subtypeData product specific typemeta.code.classobscore:ObsDataset.dataProductSubtypeVARCHARtarget_classClass of the target object as in SSAsrc.classobscore:Target.classVARCHARtarget_nameAstronomical object observed, if anymeta.id;srcobscore:Target.NameVARCHARt_stat_errorTime coord statistical errorsstat.error;timeobscore:Char.TimeAxis.Accuracy.StatError.Refval.valueDOUBLEproposal_idIdentifier of proposal to which stack belongsmeta.id;obs.proposalobscore:Provenance.Proposal.identifierVARCHARs_xel1Number of elements along the first spatial axismeta.numberobscore:Char.SpatialAxis.numBins1BIGINTprincipals_xel2Number of elements along the second spatial axismeta.numberobscore:Char.SpatialAxis.numBins2BIGINTprincipalt_xelNumber of elements along the time axismeta.numberobscore:Char.TimeAxis.numBinsBIGINTprincipalem_xelNumber of elements along the spectral axismeta.numberobscore:Char.SpectralAxis.numBinsBIGINTprincipalpol_xelNumber of polarization samplesmeta.numberobscore:Char.PolarizationAxis.numBinsBIGINTprincipal