IX/70 Chandra Source Catalog Release 2 (CSC 2.1) (Evans+, 2024)
Chandra Source Catalog Release 2 (CSC 2.1).
Evans I.N., Evans J.D., Martinez-Galarza J.R., Miller J.B., Primini F.A.,
Azadi M., Burke D.J,. Civano F.M,. D'Abrusco R., Fabbiano G.,
Graessle D.E., Grier J.D., Houck J.C., Lauer J., McCollough M.L.,
Nowak M.A., Plummer D.A., Rots A.H., Siemiginowska A., Tibbetts M.S.
<Astrophys. J. Suppl. Ser.,, 274, 22 (2024)>
=2024ApJS..274...22E 2024ApJS..274...22E
=2024yCat.9070....0E 2024yCat.9070....0E
ADC_Keywords: X-ray sources ; Surveys
Mission_Name: Chandra
Keywords: catalogs - X-rays: general
Abstract:
The Chandra Source Catalog (CSC) is a virtual X-ray astrophysics
facility that enables both detailed individual source studies and
statistical studies of large samples of X-ray sources detected in
Advanced CCD Imaging Spectrometer and High Resolution Camera-I imaging
observations obtained by the Chandra X-ray Observatory. The catalog
provides carefully curated, high-quality, and uniformly calibrated and
analyzed tabulated positional, spatial, photometric, spectral, and
temporal source properties, as well as science-ready X-ray data
products. The latter includes multiple types of source- and
field-based FITS format products that can be used as a basis for
further research, significantly simplifying follow-up analysis of
scientifically meaningful source samples. We discuss in detail the
algorithms used for the CSC Release 2 Series, including CSC 2.0, which
includes 317,167 unique X-ray sources on the sky identified in
observations released publicly through the end of 2014, and CSC 2.1,
which adds Chandra data released through the end of 2021 and expands
the catalog to 407,806 sources. Besides adding more recent
observations, the CSC Release 2 Series includes multiple algorithmic
enhancements that provide significant improvements over earlier
releases. The compact source sensitivity limit for most observations
is ∼5 photons over most of the field of view, which is ∼2x
fainter than Release 1, achieved by coadding observations and using an
optimized source detection approach. A Bayesian X-ray aperture
photometry code produces robust fluxes even in crowded fields and for
low-count sources. The current release, CSC 2.1, is tied to the
Gaia-CRF3 astrometric reference frame for the best sky positions for
catalog sources.
Description:
The Chandra Source Catalog version 2.1 (CSC 2.1) was released on April
2nd 2024; the current minor release is version 2.1.1, updated on 2024
October 18 (for more information see the Catalog Version History). It
includes measured properties for 407,806 unique compact and extended
X-ray sources and more than 1.3 million individual detections observed
with either ACIS or HRC-I observations released publicly prior to the
end of 2021. The total sky coverage is ∼730 square degrees. CSC 2.1
consists of two types of data products: database tables (e.g.
positions, significance, fluxes, hardness ratios, and variability
indices) and file-based data products (e.g. images, PHA spectra, light
curves, and sensitivity maps). Figure 1 shows the location of the
observations in CSC 2.1. The DOI for the catalog is: doi:10.25574/csc2
See more on https://cxc.cfa.harvard.edu/csc/.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
csc21mas.dat 4147 407806 Chandra Source Catalog version 2.1
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See also:
https://cxc.cfa.harvard.edu/csc/versions.html : Chandra Home Page
Byte-by-byte Description of file: csc21mas.dat
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Bytes Format Units Label Explanations
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1- 22 A22 --- 2CXO Source name, 2CXO JHHMMSS.s+DDMMSSAX
(name)
24- 46 F23.19 deg RAdeg ? Source position, ICRS right ascension
(ra)
48- 70 E23.20 deg DEdeg ? Source position, ICRS declination (dec)
72- 80 F9.5 deg GLON ? Source position, Galactic longitude
(J2000.0) (gal_l)
82- 90 F9.5 deg GLAT ? Source position, Galactic latitude
(J2000.0) (gal_b)
92- 96 F5.2 arcsec r0 ? Major radius of the 95% confidence
level position error ellipse
(errellipser0)
98- 102 F5.2 arcsec r1 ? Minor radius of the 95% confidence
level position error ellipse
(errellipser1)
104- 108 F5.1 deg PA ? Position angle (ref. local true north)
of the major axis of the 95% confidence
level error ellipse (errellipseang)
110- 117 F8.2 --- signi ? Highest flux significance (S/N) across
all stacked observations and energy
bands (significance)
119- 141 E23.18 --- like ? Highest detection log likelihood across
all stacked observations and energy
bands (likelihood)
143- 150 A8 --- likeClass Highest detection likelihood
classification across all stacked
observations and energy bands
(likelihood_class)
152- 156 A5 --- fc Source may be confused (source regions
overlap in one or more contributing
stacked observations) (conf_flag)
158- 162 A5 --- fd Highest 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
observations (ditherwarningflag)
164- 168 A5 --- fe Source is extended, or deconvolved source
extent is inconsistent with a point
source at the 90% confidence level in
one or more observations and energy
bands (extent_flag)
170- 174 A5 --- fp ACIS pile-up fraction exceeds ∼10% in all
observations; source properties may be
affected (pileup_flag)
176- 180 A5 --- fs Source is saturated in all observations;
source properties are unreliable
(satsrcflag)
182- 186 A5 --- fst Source is located on an ACIS readout
streak in all observations; source
properties may be affected
(streaksrcflag)
188- 192 A5 --- fv Source displays flux variability within
one or more observations, or between
observations, in one or more energy
bands (var_flag)
194- 198 A5 --- fvi Source hardness ratios are statistically
inconsistent between two or more
observations (varinterhard_flag)
200- 204 A5 --- fa Source was manually added in the catalog
via human review (manaddflag)
206- 210 A5 --- fi Source was manually included in the
catalog via human review (detection was
rejected by automated criteria)
(manincflag)
212- 216 A5 --- fm Source detections were manually matched
between overlapping stacked observations
via human review (manmatchflag)
218- 222 A5 --- ff Best fit source position was manually
modified via human review (manposflag)
224- 228 A5 --- fr Source region parameters (dimensions,
initial guess position input to the
Maximum Likelihood Estimator fit) were
manually modified via human review
(manregflag)
230- 236 F7.3 arcsec majb ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent; ACIS broad (0.5-7.0keV)
energy band (majoraxisb)
238- 244 F7.3 arcsec b_majb ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); ACIS broad (0.5-7.0keV) energy
band (majoraxislolim_b)
246- 252 F7.3 arcsec B_majb ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% upper confidence
limit); ACIS broad (0.5-7.0keV) energy
band (majoraxishilim_b)
254- 260 F7.3 arcsec minb ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent; ACIS broad (0.5-7.0keV)
energy band (minoraxisb)
262- 268 F7.3 arcsec b_minb ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); ACIS broad (0.5-7.0keV) energy
band (minoraxislolim_b)
270- 276 F7.3 arcsec B_minb ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent (68% upper confidence
limit); ACIS broad (0.5-7.0keV) energy
band (minoraxishilim_b)
278- 280 F3.1 deg PAb ? Position angle (ref. local true north)
of the major axis of the ellipse
defining the deconvolved source extent;
ACIS broad (0.5-7.0keV) energy band
(posangleb)
282- 290 E9.7 arcsec+2 Areab ? Area of the deconvolved source extent
ellipse, or area of the source polygon
for extended sources; ACIS broad
(0.5-7.0keV) energy band (srcareab)
292- 298 F7.3 arcsec majh ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent; ACIS hard (2.0-7.0keV)
energy band (majoraxish)
300- 306 F7.3 arcsec b_majh ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); ACIS hard (2.0-7.0keV) energy
band (majoraxislolim_h)
308- 314 F7.3 arcsec B_majh ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% upper confidence
limit); ACIS hard (2.0-7.0keV) energy
band (majoraxishilim_h)
316- 322 F7.3 arcsec minh ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent; ACIS hard (2.0-7.0keV)
energy band (minoraxish)
324- 330 F7.3 arcsec b_minh ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); ACIS hard (2.0-7.0keV) energy
band (minoraxislolim_h)
332- 338 F7.3 arcsec B_minh ? 1 sigma radius along the minor axis
of the ellipse defining the deconvolved
source extent (68% upper confidence
limit); ACIS hard (2.0-7.0keV) energy
band (minoraxishilim_h)
340- 342 F3.1 deg PAh ? Position angle (ref. local true north)
of the major axis of the ellipse
defining the deconvolved source extent;
ACIS hard (2.0-7.0keV) energy band
(posangleh)
344- 352 E9.7 arcsec+2 Areah ? Area of the deconvolved source extent
ellipse, or area of the source polygon
for extended sources; ACIS hard
(2.0-7.0keV) energy band (srcareah)
354- 360 F7.3 arcsec majm ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent; ACIS medium (1.2-2.0keV)
energy band (majoraxism)
362- 368 F7.3 arcsec b_majm ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); ACIS medium (1.2-2.0keV) energy
band (majoraxislolim_m)
370- 376 F7.3 arcsec B_majm ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% upper confidence
limit); ACIS medium (1.2-2.0keV) energy
band (majoraxishilim_m)
378- 384 F7.3 arcsec minm ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent; ACIS medium (1.2-2.0keV)
energy band (minoraxism)
386- 392 F7.3 arcsec b_minm ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); ACIS medium (1.2-2.0keV) energy
band (minoraxislolim_m)
394- 400 F7.3 arcsec B_minm ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent (68% upper confidence
limit); ACIS medium (1.2-2.0keV) energy
band (minoraxishilim_m)
402- 404 F3.1 deg PAm ? Position angle (ref. local true north)
of the major axis of the ellipse
defining the deconvolved source extent;
ACIS medium (1.2-2.0keV) energy band
(posanglem)
406- 414 E9.7 arcsec+2 Aream ? Area of the deconvolved source extent
ellipse, or area of the source polygon
for extended sources; ACIS medium
(1.2-2.0keV) energy band (srcaream)
416- 422 F7.3 arcsec majs ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent; ACIS soft (0.5-1.2keV)
energy band (majoraxiss)
424- 430 F7.3 arcsec b_majs ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); ACIS soft (0.5-1.2keV) energy
band (majoraxislolim_s)
432- 438 F7.3 arcsec B_majs ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% upper confidence
limit); ACIS soft (0.5-1.2keV) energy
band (majoraxishilim_s)
440- 446 F7.3 arcsec mins ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent; ACIS soft (0.5-1.2keV)
energy band (minoraxiss)
448- 454 F7.3 arcsec b_mins ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); ACIS soft (0.5-1.2keV) energy
band (minoraxislolim_s)
456- 462 F7.3 arcsec B_mins ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent (68% upper confidence
limit); ACIS soft (0.5-1.2keV) energy
band (minoraxishilim_s)
464- 466 F3.1 deg PAs ? Position angle (ref. local true north)
of the major axis of the ellipse
defining the deconvolved source extent;
ACIS soft (0.5-1.2keV) energy band
(posangles)
468- 476 E9.7 arcsec+2 Areas ? Area of the deconvolved source extent
ellipse, or area of the source polygon
for extended sources; ACIS soft
(0.5-1.2keV) energy band (srcareas)
478- 484 F7.3 arcsec maju ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent; ACIS ultrasoft
(0.2-0.5keV) energy band (majoraxisu)
486- 492 F7.3 arcsec b_maju ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); ACIS ultrasoft (0.2-0.5keV)
energy band (majoraxislolim_u)
494- 500 F7.3 arcsec B_maju ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% upper confidence
limit); ACIS ultrasoft (0.2-0.5keV)
energy band (majoraxishilim_u)
502- 508 F7.3 arcsec minu ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent; ACIS ultrasoft
(0.2-0.5keV) energy band (minoraxisu)
510- 516 F7.3 arcsec b_minu ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); ACIS ultrasoft (0.2-0.5keV)
energy band (minoraxislolim_u)
518- 524 F7.3 arcsec B_minu ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent (68% upper confidence
limit); ACIS ultrasoft (0.2-0.5keV)
energy band (minoraxishilim_u)
526- 528 F3.1 deg PAu ? Position angle (ref. local true north)
of the major axis of the ellipse
defining the deconvolved source extent;
ACIS ultrasoft (0.2-0.5keV) energy band
(posangleu)
530- 538 E9.6 arcsec+2 Areau ? Area of the deconvolved source extent
ellipse, or area of the source polygon
for extended sources; ACIS ultrasoft
(0.2-0.5keV) energy band (srcareau)
540- 546 F7.3 arcsec majw ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent; HRC wide (∼0.1-10.0keV)
energy band (majoraxisw)
548- 554 F7.3 arcsec b_majw ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); HRC wide (∼0.1-10.0keV) energy
band (majoraxislolim_w)
556- 562 F7.3 arcsec B_majw ? 1 sigma radius along the major axis of
the ellipse defining the deconvolved
source extent (68% upper confidence
limit); HRC wide (∼0.1-10.0keV) energy
band (majoraxishilim_w)
564- 570 F7.3 arcsec minw ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent; HRC wide (∼0.1-10.0keV)
energy band (minoraxisw)
572- 578 F7.3 arcsec b_minw ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent (68% lower confidence
limit); HRC wide (∼0.1-10.0keV) energy
band (minoraxislolim_w)
580- 586 F7.3 arcsec B_minw ? 1 sigma radius along the minor axis of
the ellipse defining the deconvolved
source extent (68% upper confidence
limit); HRC wide (∼0.1-10.0keV) energy
band (minoraxishilim_w)
588- 590 F3.1 deg PAw ? Position angle (ref. local true north)
of the major axis of the ellipse
defining the deconvolved source extent;
HRC wide (∼0.1-10.0keV) energy band
(posanglew)
592- 600 E9.6 arcsec+2 Areaw ? Area of the deconvolved source extent
ellipse, or area of the source polygon
for extended sources; HRC wide
(∼0.1-10.0keV) energy band (srcareaw)
602- 609 E8.6 ph/s/cm+2 PFluxb ? Aperture-corrected net photon flux
inferred from the source region
aperture, ACIS broad (0.5-7.0keV)
energy band (photfluxaperb) (1)
611- 618 E8.6 ph/s/cm+2 b_PFluxb ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS broad (0.5-7.0keV) energy band
(photfluxaperlolim_b) (1)
620- 627 E8.6 ph/s/cm+2 B_PFluxb ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS broad (0.5-7.0keV) energy band (1)
(photfluxaperhilim_b)
629- 636 E8.6 ph/s/cm+2 PFluxh ? Aperture-corrected net photon flux
inferred from the source region
aperture, ACIS hard (2.0-7.0keV) energy
band (photfluxaperh) (1)
638- 645 E8.6 ph/s/cm+2 b_PFluxh ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS hard (2.0-7.0keV) energy band
(photfluxaperlolim_h) (1)
647- 654 E8.6 ph/s/cm+2 B_PFluxh ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS hard (2.0-7.0keV) energy band
(photfluxaperhilim_h) (1)
656- 663 E8.6 ph/s/cm+2 PFluxm ? Aperture-corrected net photon flux
inferred from the source region
aperture, ACIS medium (1.2-2.0keV)
energy band (photfluxaperm) (1)
665- 672 E8.6 ph/s/cm+2 b_PFluxm ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS medium (1.2-2.0keV) energy band
(photfluxaperlolim_m) (1)
674- 681 E8.6 ph/s/cm+2 B_PFluxm ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS medium (1.2-2.0keV) energy band
(photfluxaperhilim_m) (1)
683- 690 E8.6 ph/s/cm+2 PFluxs ? Aperture-corrected net photon flux
inferred from the source region
aperture, ACIS soft (0.5-1.2keV) energy
band (photfluxapers) (1)
692- 699 E8.6 ph/s/cm+2 b_PFluxs ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS soft (0.5-1.2keV) energy band
(photfluxaperlolim_s) (1)
701- 708 E8.6 ph/s/cm+2 B_PFluxs ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS soft (0.5-1.2keV) energy band
(photfluxaperhilim_s) (1)
710- 717 E8.6 ph/s/cm+2 PFluxu ? Aperture-corrected net photon flux
inferred from the source region
aperture, ACIS ultrasoft (0.2-0.5keV)
energy band (photfluxaperu) (1)
719- 726 E8.6 ph/s/cm+2 b_PFluxu ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(photfluxaperlolim_u) (1)
728- 735 E8.6 ph/s/cm+2 B_PFluxu ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(photfluxaperhilim_u) (1)
737- 744 E8.6 ph/s/cm+2 PFluxw ? Aperture-corrected net photon flux
inferred from the source region
aperture, HRC wide (∼0.1-10.0keV) energy
band (photfluxaperw) (1)
746- 753 E8.6 ph/s/cm+2 b_PFluxw ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(photfluxaperlolim_w) (1)
755- 762 E8.6 ph/s/cm+2 B_PFluxw ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(photfluxaperhilim_w) (1)
764- 771 E8.6 ph/s/cm+2 PFavgb ? Aperture-corrected net photon flux
inferred from the source region
aperture, ACIS broad (0.5-7.0keV)
energy band (photfluxaperavg_b) (2)
773- 780 E8.6 ph/s/cm+2 b_PFavgb ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS broad (0.5-7.0keV) energy band
(photfluxaperavglolimb) (2)
782- 789 E8.6 ph/s/cm+2 B_PFavgb ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS broad (0.5-7.0keV) energy band
(photfluxaperavghilimb) (2)
791- 798 E8.6 ph/s/cm+2 PFavgh ? Aperture-corrected net photon flux
inferred from the source region
aperture, ACIS hard (2.0-7.0keV)
energy band (photfluxaperavg_h) (2)
800- 807 E8.6 ph/s/cm+2 b_PFavgh ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS hard (2.0-7.0keV) energy band
(photfluxaperavglolimh) (2)
809- 816 E8.6 ph/s/cm+2 B_PFavgh ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS hard (2.0-7.0keV) energy band
(photfluxaperavghilimh) (2)
818- 825 E8.6 ph/s/cm+2 PFavgm ? Aperture-corrected net photon flux
inferred from the source region
aperture, ACIS medium (1.2-2.0keV)
energy band (photfluxaperavg_m) (2)
827- 834 E8.6 ph/s/cm+2 b_PFavgm ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS medium (1.2-2.0keV) energy band
(photfluxaperavglolimm) (2)
836- 843 E8.6 ph/s/cm+2 B_PFavgm ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS medium (1.2-2.0keV) energy band
(photfluxaperavghilimm) (2)
845- 852 E8.6 ph/s/cm+2 PFavgs ? Aperture-corrected net photon flux
inferred from the source region
aperture, ACIS soft (0.5-1.2keV)
energy band (photfluxaperavg_s) (2)
854- 861 E8.6 ph/s/cm+2 b_PFavgs ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS soft (0.5-1.2keV) energy band
(photfluxaperavglolims) (2)
863- 870 E8.6 ph/s/cm+2 B_PFavgs ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS soft (0.5-1.2keV) energy band
(photfluxaperavghilims) (2)
872- 879 E8.6 ph/s/cm+2 PFavgu ? Aperture-corrected net photon flux
inferred from the source region
aperture; ACIS ultrasoft (0.2-0.5keV)
energy band (photfluxaperavg_u) (2)
881- 888 E8.6 ph/s/cm+2 b_PFavgu ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(photfluxaperavglolimu) (2)
890- 897 E8.6 ph/s/cm+2 B_PFavgu ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(photfluxaperavghilimu) (2)
899- 906 E8.6 ph/s/cm+2 PFavgw ? Aperture-corrected net photon flux
inferred from the source region
aperture, HRC wide (∼0.1-10.0keV)
energy band (photfluxaperavg_w) (2)
908- 915 E8.6 ph/s/cm+2 b_PFavgw ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% lower confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(photfluxaperavglolimw) (2)
917- 924 E8.6 ph/s/cm+2 B_PFavgw ? Aperture-corrected net photon flux
inferred from the source region
aperture (68% upper confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(photfluxaperavghilimw) (2)
926- 933 E8.3 mW/m2 Fluxb ? Aperture-corrected net energy flux
inferred from the source region
aperture, ACIS broad (0.5-7.0keV) energy
band (fluxaperb) (1)
935- 942 E8.3 mW/m2 b_Fluxb ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS broad (0.5-7.0keV) energy band
(fluxaperlolim_b) (1)
944- 951 E8.3 mW/m2 B_Fluxb ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS broad (0.5-7.0keV) energy band
(fluxaperhilim_b) (1)
953- 960 E8.3 mW/m2 Fluxh ? Aperture-corrected net energy flux
inferred from the source region
aperture, ACIS hard (2.0-7.0keV) energy
band (fluxaperh) (1)
962- 969 E8.3 mW/m2 b_Fluxh ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS hard (2.0-7.0keV) energy band
(fluxaperlolim_h) (1)
971- 978 E8.3 mW/m2 B_Fluxh ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS hard (2.0-7.0keV) energy band
(fluxaperhilim_h) (1)
980- 987 E8.3 mW/m2 Fluxm ? Aperture-corrected net energy flux
inferred from the source region
aperture, ACIS medium (1.2-2.0keV)
energy band (fluxaperm) (1)
989- 996 E8.3 mW/m2 b_Fluxm ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS medium (1.2-2.0keV) energy band
(fluxaperlolim_m) (1)
998-1005 E8.3 mW/m2 B_Fluxm ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS medium (1.2-2.0keV) energy band
(fluxaperhilim_m) (1)
1007-1014 E8.3 mW/m2 Fluxs ? Aperture-corrected net energy flux
inferred from the source region
aperture, ACIS soft (0.5-1.2keV) energy
band (fluxapers) (1)
1016-1023 E8.3 mW/m2 b_Fluxs ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS soft (0.5-1.2keV) energy band
(fluxaperlolim_s) (1)
1025-1032 E8.3 mW/m2 B_Fluxs ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS soft (0.5-1.2keV) energy band
(fluxaperhilim_s) (1)
1034-1041 E8.6 mW/m2 Fluxu ? Aperture-corrected net energy flux
inferred from the source region
aperture, ACIS ultrasoft (0.2-0.5keV)
energy band (fluxaperu) (1)
1043-1050 E8.6 mW/m2 b_Fluxu ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxaperlolim_u) (1)
1052-1059 E8.6 mW/m2 B_Fluxu ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxaperhilim_u) (1)
1061-1068 E8.3 mW/m2 Fluxw ? Aperture-corrected net energy flux
inferred from the source region
aperture, HRC wide (∼0.1-10.0keV) energy
band (fluxaperw) (1)
1070-1077 E8.3 mW/m2 b_Fluxw ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxaperlolim_w) (1)
1079-1086 E8.3 mW/m2 B_Fluxw ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxaperhilim_w)
1088-1095 E8.3 mW/m2 Favgb ? Aperture-corrected net energy flux
inferred from the source region
aperture, ACIS broad (0.5-7.0keV) energy
band (fluxaperavg_b) (2)
1097-1104 E8.3 mW/m2 b_Favgb ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS broad (0.5-7.0keV) energy band
(fluxaperavglolimb) (2)
1106-1113 E8.3 mW/m2 B_Favgb ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS broad (0.5-7.0keV) energy band
(fluxaperavghilimb) (2)
1115-1122 E8.3 mW/m2 Favgh ? Aperture-corrected net energy flux
inferred from the source region
aperture ; ACIS hard (2.0-7.0keV)
energy band (fluxaperavg_h) (2)
1124-1131 E8.3 mW/m2 b_Favgh ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS hard (2.0-7.0keV) energy band
(fluxaperavglolimh) (2)
1133-1140 E8.3 mW/m2 B_Favgh ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS hard (2.0-7.0keV) energy band
(fluxaperavghilimh) (2)
1142-1149 E8.3 mW/m2 Favgm ? Aperture-corrected net energy flux
inferred from the source region
aperture, ACIS medium (1.2-2.0keV)
energy band (fluxaperavg_m) (2)
1151-1158 E8.3 mW/m2 b_Favgm ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS medium (1.2-2.0keV) energy band
(fluxaperavglolimm) (2)
1160-1167 E8.3 mW/m2 B_Favgm ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS medium (1.2-2.0keV) energy band
(fluxaperavghilimm) (2)
1169-1176 E8.3 mW/m2 Favgs ? Aperture-corrected net energy flux
inferred from the source region
aperture ACIS soft (0.5-1.2keV)
energy band (fluxaperavg_s) (2)
1178-1185 E8.3 mW/m2 b_Favgs ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS soft (0.5-1.2keV) energy band
(fluxaperavglolims) (2)
1187-1194 E8.3 mW/m2 B_Favgs ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS soft (0.5-1.2keV) energy band
(fluxaperavghilims) (2)
1196-1203 E8.6 mW/m2 Favgu ? Aperture-corrected net energy flux
inferred from the source region
aperture ; ACIS ultrasoft (0.2-0.5keV)
energy band (fluxaperavg_u) (2)
1205-1212 E8.6 mW/m2 b_Favgu ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxaperavglolimu) (2)
1214-1221 E8.6 mW/m2 B_Favgu ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxaperavghilimu) (2)
1223-1230 E8.3 mW/m2 Favgw ? Aperture-corrected net energy flux
inferred from the source region
aperture; HRC wide (∼0.1-10.0keV)
energy band (fluxaperavg_w) (2)
1232-1239 E8.3 mW/m2 b_Favgw ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% lower confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxaperavglolimw) (2)
1241-1248 E8.3 mW/m2 B_Favgw ? Aperture-corrected net energy flux
inferred from the source region
aperture (68% upper confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxaperavghilimw) (2)
1250-1257 E8.6 ph/s/cm+2 PF90b ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
ACIS broad (0.5-7.0keV) energy band
(photfluxaper90b) (1)
1259-1266 E8.6 ph/s/cm+2 b_PF90b ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS broad
(0.5-7.0keV) energy band
(photfluxaper90lolim_b) (1)
1268-1275 E8.6 ph/s/cm+2 B_PF90b ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS broad
(0.5-7.0keV) energy band
(photfluxaper90hilim_b) (1)
1277-1284 E8.6 ph/s/cm+2 PF90h ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
ACIS hard (2.0-7.0keV) energy band
(photfluxaper90h) (1)
1286-1293 E8.6 ph/s/cm+2 b_PF90h ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS hard
(2.0-7.0keV) energy band
(photfluxaper90lolim_h) (1)
1295-1302 E8.6 ph/s/cm+2 B_PF90h ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS hard
(2.0-7.0keV) energy band
(photfluxaper90hilim_h) (1)
1304-1311 E8.6 ph/s/cm+2 PF90m ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
ACIS medium (1.2-2.0keV) energy band
(photfluxaper90m) (1)
1313-1320 E8.6 ph/s/cm+2 b_PF90m ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS
medium (1.2-2.0keV) energy band
(photfluxaper90lolim_m) (1)
1322-1329 E8.6 ph/s/cm+2 B_PF90m ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS
medium (1.2-2.0keV) energy band
(photfluxaper90hilim_m) (1)
1331-1338 E8.6 ph/s/cm+2 PF90s ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
ACIS soft (0.5-1.2keV) energy band
(photfluxaper90s) (1)
1340-1347 E8.6 ph/s/cm+2 b_PF90s ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS soft
(0.5-1.2keV) energy band
(photfluxaper90lolim_s) (1)
1349-1356 E8.6 ph/s/cm+2 B_PF90s ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS soft
(0.5-1.2keV) energy band
(photfluxaper90hilim_s) (1)
1358-1365 E8.6 ph/s/cm+2 PF90u ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
ACIS ultrasoft (0.2-0.5keV) energy band
(photfluxaper90u) (1)
1367-1374 E8.6 ph/s/cm+2 b_PF90u ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS
ultrasoft (0.2-0.5keV) energy band
(photfluxaper90lolim_u) (1)
1376-1383 E8.6 ph/s/cm+2 B_PF90u ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS
ultrasoft (0.2-0.5keV) energy band
(photfluxaper90hilim_u) (1)
1385-1392 E8.6 ph/s/cm+2 PF90w ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
HRC wide (∼0.1-10.0keV) energy band
(photfluxaper90w) (1)
1394-1401 E8.6 ph/s/cm+2 b_PF90w ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); HRC wide
(∼0.1-10.0keV) energy band
(photfluxaper90lolim_w) (1)
1403-1410 E8.6 ph/s/cm+2 B_PF90w ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); HRC wide
(∼0.1-10.0keV) energy band
(photfluxaper90hilim_w) (1)
1412-1419 E8.6 ph/s/cm+2 PF90avgb ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
ACIS broad (0.5-7.0keV) energy band
(photfluxaper90avg_b) (2)
1421-1428 E8.6 ph/s/cm+2 b_PF90avgb ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS broad
(0.5-7.0keV) energy band
(photfluxaper90avglolimb) (2)
1430-1437 E8.6 ph/s/cm+2 B_PF90avgb ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS broad
(0.5-7.0keV) energy band
(photfluxaper90avghilimb) (2)
1439-1446 E8.6 ph/s/cm+2 PF90avgh ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
ACIS hard (2.0-7.0keV) energy band
(photfluxaper90avg_h) (2)
1448-1455 E8.6 ph/s/cm+2 b_PF90avgh ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS hard
(2.0-7.0keV) energy band
(photfluxaper90avglolimh) (2)
1457-1464 E8.6 ph/s/cm+2 B_PF90avgh ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS hard
(2.0-7.0keV) energy band
(photfluxaper90avghilimh) (2)
1466-1473 E8.6 ph/s/cm+2 PF90avgm ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
ACIS medium (1.2-2.0keV) energy band
(photfluxaper90avg_m) (2)
1475-1482 E8.6 ph/s/cm+2 b_PF90avgm ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS
medium (1.2-2.0keV) energy band
(photfluxaper90avglolimm) (2)
1484-1491 E8.6 ph/s/cm+2 B_PF90avgm ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS
medium (1.2-2.0keV) energy band
(photfluxaper90avghilimm) (2)
1493-1500 E8.6 ph/s/cm+2 PF90avgs ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
ACIS soft (0.5-1.2keV) energy band
(photfluxaper90avg_s) (2)
1502-1509 E8.6 ph/s/cm+2 b_PF90avgs ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS soft
(0.5-1.2keV) energy band
(photfluxaper90avglolims) (2)
1511-1518 E8.6 ph/s/cm+2 B_PF90avgs ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS soft
(0.5-1.2keV) energy band
(photfluxaper90avghilims) (2)
1520-1527 E8.6 ph/s/cm+2 PF90avgu ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
ACIS ultrasoft (0.2-0.5keV) energy band
(photfluxaper90avg_u) (2)
1529-1536 E8.6 ph/s/cm+2 b_PF90avgu ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS
ultrasoft (0.2-0.5keV) energy band
(photfluxaper90avglolimu) (2)
1538-1545 E8.6 ph/s/cm+2 B_PF90avgu ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS
ultrasoft (0.2-0.5keV) energy band
(photfluxaper90avghilimu) (2)
1547-1554 E8.6 ph/s/cm+2 PF90avgw ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
HRC wide (∼0.1-10.0keV) energy band
(photfluxaper90avg_w) (2)
1556-1563 E8.6 ph/s/cm+2 b_PF90avgw ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); HRC wide
(∼0.1-10.0keV) energy band
(photfluxaper90avglolimw) (2)
1565-1572 E8.6 ph/s/cm+2 B_PF90avgw ? Aperture-corrected net photon flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); HRC wide
(∼0.1-10.0keV) energy band
(photfluxaper90avghilimw) (2)
1574-1581 E8.3 mW/m2 F90b ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
ACIS broad (0.5-7.0keV) energy band
(fluxaper90b) (1)
1583-1590 E8.3 mW/m2 b_F90b ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS broad
(0.5-7.0keV) energy band
(fluxaper90lolim_b) (2)
1592-1599 E8.3 mW/m2 B_F90b ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS broad
(0.5-7.0keV) energy band
(fluxaper90hilim_b) (1)
1601-1608 E8.3 mW/m2 F90h ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
ACIS hard (2.0-7.0keV) energy band
(fluxaper90h) (1)
1610-1617 E8.3 mW/m2 b_F90h ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS hard
(2.0-7.0keV) energy band
(fluxaper90lolim_h) (1)
1619-1626 E8.3 mW/m2 B_F90h ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS hard
(2.0-7.0keV) energy band
(fluxaper90hilim_h) (1)
1628-1635 E8.3 mW/m2 F90m ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
ACIS medium (1.2-2.0keV) energy band
(fluxaper90m) (1)
1637-1644 E8.3 mW/m2 b_F90m ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS
medium (1.2-2.0keV) energy band
(fluxaper90lolim_m) (1)
1646-1653 E8.3 mW/m2 B_F90m ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS
medium (1.2-2.0keV) energy band
(fluxaper90hilim_m) (1)
1655-1662 E8.3 mW/m2 F90s ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
ACIS soft (0.5-1.2keV) energy band
(fluxaper90s) (1)
1664-1671 E8.3 mW/m2 b_F90s ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS soft
(0.5-1.2keV) energy band
(fluxaper90lolim_s) (1)
1673-1680 E8.3 mW/m2 B_F90s ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS soft
(0.5-1.2keV) energy band
(fluxaper90hilim_s) (1)
1682-1689 E8.6 mW/m2 F90u ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxaper90u) (1)
1691-1698 E8.6 mW/m2 b_F90u ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS
ultrasoft (0.2-0.5keV) energy band
(fluxaper90lolim_u) (1)
1700-1707 E8.6 mW/m2 B_F90u ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS
ultrasoft (0.2-0.5keV) energy band
(fluxaper90hilim_u) (1)
1709-1716 E8.3 mW/m2 F90w ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
HRC wide (∼0.1-10.0keV) energy band
(fluxaper90w) (1)
1718-1725 E8.3 mW/m2 b_F90w ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); HRC wide
(∼0.1-10.0keV) energy band
(fluxaper90lolim_w) (1)
1727-1734 E8.3 mW/m2 B_F90w ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); HRC wide
(∼0.1-10.0keV) energy band
(fluxaper90hilim_w) (1)
1736-1743 E8.3 mW/m2 EF90avgb ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
ACIS broad (0.5-7.0keV) energy band
(fluxaper90avg_b) (2)
1745-1752 E8.3 mW/m2 b_EF90avgb ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS broad
(0.5-7.0keV) energy band
(fluxaper90avglolimb) (2)
1754-1761 E8.3 mW/m2 B_EF90avgb ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS broad
(0.5-7.0keV) energy band
(fluxaper90avghilimb) (2)
1763-1770 E8.3 mW/m2 EF90avgh ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
ACIS hard (2.0-7.0keV) energy band
(fluxaper90avg_h) (2)
1772-1779 E8.3 mW/m2 b_EF90avgh ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS hard
(2.0-7.0keV) energy band
(fluxaper90avglolimh) (2)
1781-1788 E8.3 mW/m2 B_EF90avgh ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS hard
(2.0-7.0keV) energy band
(fluxaper90avghilimh) (2)
1790-1797 E8.3 mW/m2 EF90avgm ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
ACIS medium (1.2-2.0keV) energy band
(fluxaper90avg_m) (2)
1799-1806 E8.3 mW/m2 b_EF90avgm ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS
medium (1.2-2.0keV) energy band
(fluxaper90avglolimm) (2)
1808-1815 E8.3 mW/m2 B_EF90avgm ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS
medium (1.2-2.0keV) energy band
(fluxaper90avghilimm) (2)
1817-1824 E8.3 mW/m2 EF90avgs ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
ACIS soft (0.5-1.2keV) energy band
(fluxaper90avg_s) (2)
1826-1833 E8.3 mW/m2 b_EF90avgs ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS soft
(0.5-1.2keV) energy band
(fluxaper90avglolims) (2)
1835-1842 E8.3 mW/m2 B_EF90avgs ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); ACIS soft
(0.5-1.2keV) energy band
(fluxaper90avghilims) (2)
1844-1851 E8.6 mW/m2 EF90avgu ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxaper90avg_u) (2)
1853-1860 E8.6 mW/m2 b_EF90avgu ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% lower confidence limit); ACIS
ultrasoft (0.2-0.5keV) energy band
(fluxaper90avglolimu) (2)
1862-1869 E8.6 mW/m2 B_EF90avgu ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxaper90avghilimu) (2)
1871-1878 E8.3 mW/m2 EF90avgw ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
HRC wide (∼0.1-10.0keV) energy band
(fluxaper90avg_w) (2)
1880-1887 E8.3 mW/m2 b_EF90avgw ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
HRC wide (∼0.1-10.0keV) energy
band (fluxaper90avglolimw) (2)
1889-1896 E8.3 mW/m2 B_EF90avgw ? Aperture-corrected net energy flux
inferred from the PSF 90% ECF aperture,
(68% upper confidence limit); HRC wide
(∼0.1-10.0keV) energy band
(fluxaper90avghilimw) (2)
1898-1899 I2 --- Ns ? Number of sources fit simultaneously
to compute aperture photometry
quantities (phot_nsrcs)
1901-1908 E8.3 mW/m2 FPLb ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model
[NH=NH(Gal); Gamma=2.0];
ACIS broad (0.5-7.0keV) energy band
(fluxpowlawaper_b)
1910-1917 E8.3 mW/m2 b_FPLb ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model
[NH=NH(Gal); Gamma=2.0]
(68% lower confidence limit);
ACIS broad (0.5-7.0keV) energy band
(fluxpowlawaperlolimb)
1919-1926 E8.3 mW/m2 B_FPLb ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model
[NH=NH(Gal); Gamma=2.0]
(68% upper confidence limit);
ACIS broad (0.5-7.0keV) energy band
(fluxpowlawaperhilimb)
1928-1935 E8.3 mW/m2 FPLh ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model
[NH=NH(Gal); Gamma=2.0];
ACIS hard (2.0-7.0keV) energy band
(fluxpowlawaper_h)
1937-1944 E8.3 mW/m2 b_FPLh ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model
[NH=NH(Gal); Gamma=2.0]
(68% lower confidence limit);
ACIS hard (2.0-7.0keV) energy band
(fluxpowlawaperlolimh)
1946-1953 E8.3 mW/m2 B_FPLh ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model
[NH=NH(Gal); Gamma=2.0]
(68% upper confidence limit);
ACIS hard (2.0-7.0keV) energy band
(fluxpowlawaperhilimh)
1955-1962 E8.3 mW/m2 FPLm ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model
[NH=NH(Gal); Gamma=2.0];
ACIS medium (1.2-2.0keV) energy band
(fluxpowlawaper_m)
1964-1971 E8.3 mW/m2 b_FPLm ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model
[NH=NH(Gal); Gamma=2.0]
(68% lower confidence limit);
ACIS medium (1.2-2.0keV) energy band
(fluxpowlawaperlolimm)
1973-1980 E8.3 mW/m2 B_FPLm ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model
[NH=NH(Gal); Gamma=2.0]
(68% upper confidence limit);
ACIS medium (1.2-2.0keV) energy band
(fluxpowlawaperhilimm)
1982-1989 E8.3 mW/m2 FPLs ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model
[NH=NH(Gal); Gamma=2.0];
ACIS soft (0.5-1.2keV) energy band
(fluxpowlawaper_s)
1991-1998 E8.3 mW/m2 b_FPLs ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model [NH=NH(Gal);
Gamma=2.0] (68% lower confidence
limit); ACIS soft (0.5-1.2keV) energy
band (fluxpowlawaperlolims)
2000-2007 E8.3 mW/m2 B_FPLs ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model [NH=NH(Gal);
Gamma=2.0] (68% upper confidence
limit); ACIS soft (0.5-1.2keV) energy
band (fluxpowlawaperhilims)
2009-2016 E8.3 mW/m2 FPLu ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model [NH=NH(Gal);
Gamma=2.0]; ACIS ultrasoft
(0.2-0.5keV) energy band
(fluxpowlawaper_u)
2018-2025 E8.3 mW/m2 b_FPLu ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model [NH=NH(Gal);
Gamma=2.0] (68% lower confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxpowlawaperlolimu)
2027-2034 E8.3 mW/m2 B_FPLu ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model [NH=NH(Gal);
Gamma=2.0] (68% upper confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxpowlawaperhilimu)
2036-2043 E8.3 mW/m2 FPLw ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model [NH=NH(Gal);
Gamma=2.0]; HRC wide (∼0.1-10.0keV)
energy band (fluxpowlawaper_w)
2045-2052 E8.3 mW/m2 b_FPLw ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model [NH=NH(Gal);
Gamma=2.0] (68% lower confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxpowlawaperlolimw)
2054-2061 E8.3 mW/m2 B_FPLw ? Source region aperture model energy
flux inferred from the canonical
absorbed power law model [NH=NH(Gal);
Gamma=2.0] (68% upper confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxpowlawaperhilimw)
2063-2070 E8.3 mW/m2 FBBb ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV]; ACIS broad (0.5-7.0keV)
energy band (fluxbbaper_b)
2072-2079 E8.3 mW/m2 b_FBBb ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); ACIS broad (0.5-7.0keV) energy
band (fluxbbaperlolimb)
2081-2088 E8.3 mW/m2 B_FBBb ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); ACIS broad (0.5-7.0keV) energy
band (fluxbbaperhilimb)
2090-2097 E8.3 mW/m2 FBBh ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV]; ACIS hard (2.0-7.0keV)
energy band (fluxbbaper_h)
2099-2106 E8.3 mW/m2 b_FBBh ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); ACIS hard (2.0-7.0keV) energy
band (fluxbbaperlolimh)
2108-2115 E8.3 mW/m2 B_FBBh ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); ACIS hard (2.0-7.0keV) energy
band (fluxbbaperhilimh)
2117-2124 E8.3 mW/m2 FBBm ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV]; ACIS medium (1.2-2.0keV)
energy band (fluxbbaper_m)
2126-2133 E8.3 mW/m2 b_FBBm ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); ACIS medium (1.2-2.0keV) energy
band (fluxbbaperlolimm)
2135-2142 E8.3 mW/m2 B_FBBm ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); ACIS medium (1.2-2.0keV) energy
band (fluxbbaperhilimm)
2144-2151 E8.3 mW/m2 FBBs ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV]; ACIS soft (0.5-1.2keV)
energy band (fluxbbaper_s)
2153-2160 E8.3 mW/m2 b_FBBs ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); ACIS soft (0.5-1.2keV) energy
band (fluxbbaperlolims)
2162-2169 E8.3 mW/m2 B_FBBs ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); ACIS soft (0.5-1.2keV) energy
band (fluxbbaperhilims)
2171-2178 E8.3 mW/m2 FBBu ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV]; ACIS ultrasoft
(0.2-0.5keV) energy band
(fluxbbaper_u)
2180-2187 E8.3 mW/m2 b_FBBu ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); ACIS ultrasoft (0.2-0.5keV)
energy band (fluxbbaperlolimu)
2189-2196 E8.3 mW/m2 B_FBBu ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); ACIS ultrasoft (0.2-0.5keV)
energy band (fluxbbaperhilimu)
2198-2205 E8.3 mW/m2 FBBw ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV]; HRC wide (∼0.1-10.0keV)
energy band (fluxbbaper_w)
2207-2214 E8.3 mW/m2 b_FBBw ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); HRC wide (∼0.1-10.0keV) energy
band (fluxbbaperlolimw)
2216-2223 E8.3 mW/m2 B_FBBw ? Source region aperture model energy
flux inferred from the canonical
absorbed black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); HRC wide (∼0.1-10.0keV) energy
band (fluxbbaperhilimw)
2225-2232 E8.3 mW/m2 FBSb ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV]; ACIS broad
(0.5-7.0keV) energy band
(fluxbremsaper_b)
2234-2241 E8.3 mW/m2 b_FBSb ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% lower
confidence limit); ACIS broad
(0.5-7.0keV) energy band
(fluxbremsaperlolimb)
2243-2250 E8.3 mW/m2 B_FBSb ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% upper
confidence limit); ACIS broad
(0.5-7.0keV) energy band
(fluxbremsaperhilimb)
2252-2259 E8.3 mW/m2 FBSh ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV]; ACIS hard
(2.0-7.0keV) energy band
(fluxbremsaper_h)
2261-2268 E8.3 mW/m2 b_FBSh ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% lower
confidence limit); ACIS hard
(2.0-7.0keV) energy band
(fluxbremsaperlolimh)
2270-2277 E8.3 mW/m2 B_FBSh ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% upper
confidence limit); ACIS hard
(2.0-7.0keV) energy band
(fluxbremsaperhilimh)
2279-2286 E8.3 mW/m2 FBSm ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV];
ACIS medium (1.2-2.0keV) energy band
(fluxbremsaper_m)
2288-2295 E8.3 mW/m2 b_FBSm ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% lower
confidence limit); ACIS medium
(1.2-2.0keV) energy band
(fluxbremsaperlolimm)
2297-2304 E8.3 mW/m2 B_FBSm ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% upper
confidence limit); ACIS medium
(1.2-2.0keV) energy band
(fluxbremsaperhilimm)
2306-2313 E8.3 mW/m2 FBSs ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV]; ACIS soft
(0.5-1.2keV) energy band
(fluxbremsaper_s)
2315-2322 E8.3 mW/m2 b_FBSs ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% lower
confidence limit); ACIS soft
(0.5-1.2keV) energy band
(fluxbremsaperlolims)
2324-2331 E8.3 mW/m2 B_FBSs ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% upper
confidence limit); ACIS soft
(0.5-1.2keV) energy band
(fluxbremsaperhilims)
2333-2340 E8.3 mW/m2 FBSu ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV]; ACIS
ultrasoft (0.2-0.5keV) energy band
(fluxbremsaper_u)
2342-2349 E8.3 mW/m2 b_FBSu ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% lower
confidence limit); ACIS ultrasoft
(0.2-0.5keV) energy band
(fluxbremsaperlolimu)
2351-2358 E8.3 mW/m2 B_FBSu ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% upper
confidence limit); ACIS ultrasoft
(0.2-0.5keV) energy band
(fluxbremsaperhilimu)
2360-2367 E8.3 mW/m2 FBSw ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV]; HRC wide
(∼0.1-10.0keV) energy band
(fluxbremsaper_w)
2369-2376 E8.3 mW/m2 b_FBSw ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% lower
confidence limit); HRC wide
(∼0.1-10.0keV) energy band
(fluxbremsaperlolimw)
2378-2385 E8.3 mW/m2 B_FBSw ? Source region aperture model energy
flux inferred from the canonical
absorbed bremsstrahlung model
[NH=NH(Gal); kT=3.5keV] (68% upper
confidence limit); HRC wide
(∼0.1-10.0keV) energy band
(fluxbremsaperhilimw)
2387-2394 E8.3 mW/m2 FAPb ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV]; ACIS broad (0.5-7.0keV)
energy band (fluxapecaper_b)
2396-2403 E8.3 mW/m2 b_FAPb ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% lower confidence
limit); ACIS broad (0.5-7.0keV) energy
band (fluxapecaperlolimb)
2405-2412 E8.3 mW/m2 B_FAPb ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% upper confidence
limit); ACIS broad (0.5-7.0keV) energy
band (fluxapecaperhilimb)
2414-2421 E8.3 mW/m2 FAPh ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV]; ACIS hard (2.0-7.0keV)
energy band (fluxapecaper_h)
2423-2430 E8.3 mW/m2 b_FAPh ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% lower confidence
limit); ACIS hard (2.0-7.0keV) energy
band (fluxapecaperlolimh)
2432-2439 E8.3 mW/m2 B_FAPh ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% upper confidence
limit); ACIS hard (2.0-7.0keV) energy
band (fluxapecaperhilimh)
2441-2448 E8.3 mW/m2 FAPm ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV]; ACIS medium (1.2-2.0keV)
energy band (fluxapecaper_m)
2450-2457 E8.3 mW/m2 b_FAPm ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% lower confidence
limit); ACIS medium (1.2-2.0keV) energy
band (fluxapecaperlolimm)
2459-2466 E8.3 mW/m2 B_FAPm ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% upper confidence
limit); ACIS medium (1.2-2.0keV) energy
band (fluxapecaperhilimm)
2468-2475 E8.3 mW/m2 FAPs ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV]; ACIS soft (0.5-1.2keV)
energy band (fluxapecaper_s)
2477-2484 E8.3 mW/m2 b_FAPs ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% lower confidence
limit); ACIS soft (0.5-1.2keV) energy
band (fluxapecaperlolims)
2486-2493 E8.3 mW/m2 B_FAPs ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% upper confidence
limit); ACIS soft (0.5-1.2keV) energy
band (fluxapecaperhilims)
2495-2502 E8.3 mW/m2 FAPu ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV]; ACIS ultrasoft
(0.2-0.5keV) energy band
(fluxapecaper_u)
2504-2511 E8.3 mW/m2 b_FAPu ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% lower confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxapecaperlolimu)
2513-2520 E8.3 mW/m2 B_FAPu ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% upper confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxapecaperhilimu)
2522-2529 E8.3 mW/m2 FAPw ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV]; HRC wide (∼0.1-10.0keV)
energy band (fluxapecaper_w)
2531-2538 E8.3 mW/m2 b_FAPw ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% lower confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxapecaperlolimw)
2540-2547 E8.3 mW/m2 B_FAPw ? Source region aperture model energy
flux inferred from the canonical
absorbed APEC model [NH=NH(Gal);
kT=6.5keV] (68% upper confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxapecaperhilimw)
2549-2556 E8.3 mW/m2 FPL90b ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0]; ACIS broad (0.5-7.0keV)
energy band (fluxpowlawaper90_b)
2558-2565 E8.3 mW/m2 b_FPL90b ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% lower confidence limit);
ACIS broad (0.5-7.0keV) energy band
(fluxpowlawaper90lolimb)
2567-2574 E8.3 mW/m2 B_FPL90b ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% upper confidence limit);
ACIS broad (0.5-7.0keV) energy band
(fluxpowlawaper90hilimb)
2576-2583 E8.3 mW/m2 FPL90h ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0]; ACIS hard (2.0-7.0keV)
energy band (fluxpowlawaper90_h)
2585-2592 E8.3 mW/m2 b_FPL90h ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% lower confidence limit);
ACIS hard (2.0-7.0keV) energy band
(fluxpowlawaper90lolimh)
2594-2601 E8.3 mW/m2 B_FPL90h ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% upper confidence limit);
ACIS hard (2.0-7.0keV) energy band
(fluxpowlawaper90hilimh)
2603-2610 E8.3 mW/m2 FPL90m ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0]; ACIS medium (1.2-2.0keV)
energy band (fluxpowlawaper90_m)
2612-2619 E8.3 mW/m2 b_FPL90m ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% lower confidence limit);
ACIS medium (1.2-2.0keV) energy band
(fluxpowlawaper90lolimm)
2621-2628 E8.3 mW/m2 B_FPL90m ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% upper confidence limit);
ACIS medium (1.2-2.0keV) energy band
(fluxpowlawaper90hilimm)
2630-2637 E8.3 mW/m2 FPL90s ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0]; ACIS soft (0.5-1.2keV)
energy band (fluxpowlawaper90_s)
2639-2646 E8.3 mW/m2 b_FPL90s ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% lower confidence limit);
ACIS soft (0.5-1.2keV) energy band
(fluxpowlawaper90lolims)
2648-2655 E8.3 mW/m2 B_FPL90s ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% upper confidence limit);
ACIS soft (0.5-1.2keV) energy band
(fluxpowlawaper90hilims)
2657-2664 E8.3 mW/m2 FPL90u ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0]; ACIS ultrasoft (0.2-0.5keV)
energy band (fluxpowlawaper90_u)
2666-2673 E8.3 mW/m2 b_FPL90u ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% lower confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxpowlawaper90lolimu)
2675-2682 E8.3 mW/m2 B_FPL90u ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% upper confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxpowlawaper90hilimu)
2684-2691 E8.3 mW/m2 FPL90w ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0]; HRC wide (∼0.1-10.0keV)
energy band (fluxpowlawaper90_w)
2693-2700 E8.3 mW/m2 b_FPL90w ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% lower confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxpowlawaper90lolimw)
2702-2709 E8.3 mW/m2 B_FPL90w ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
power law model [NH=NH(Gal);
Gamma=2.0] (68% upper confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxpowlawaper90hilimw)
2711-2718 E8.3 mW/m2 FBB90b ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV]; ACIS broad (0.5-7.0keV)
energy band (fluxbbaper90_b)
2720-2727 E8.3 mW/m2 b_FBB90b ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); ACIS broad (0.5-7.0keV) energy
band (fluxbbaper90lolimb)
2729-2736 E8.3 mW/m2 B_FBB90b ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); ACIS broad (0.5-7.0keV) energy
band (fluxbbaper90hilimb)
2738-2745 E8.3 mW/m2 FBB90h ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV]; ACIS hard (2.0-7.0keV)
energy band (fluxbbaper90_h)
2747-2754 E8.3 mW/m2 b_FBB90h ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); ACIS hard (2.0-7.0keV) energy
band (fluxbbaper90lolimh)
2756-2763 E8.3 mW/m2 B_FBB90h ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); ACIS hard (2.0-7.0keV) energy
band (fluxbbaper90hilimh)
2765-2772 E8.3 mW/m2 FBB90m ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV]; ACIS medium (1.2-2.0keV)
energy band (fluxbbaper90_m)
2774-2781 E8.3 mW/m2 b_FBB90m ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); ACIS medium (1.2-2.0keV)
energy band (fluxbbaper90lolimm)
2783-2790 E8.3 mW/m2 B_FBB90m ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); ACIS medium (1.2-2.0keV) energy
band (fluxbbaper90hilimm)
2792-2799 E8.3 mW/m2 FBB90s ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV]; ACIS soft (0.5-1.2keV)
energy band (fluxbbaper90_s)
2801-2808 E8.3 mW/m2 b_FBB90s ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); ACIS soft (0.5-1.2keV) energy
band (fluxbbaper90lolims)
2810-2817 E8.3 mW/m2 B_FBB90s ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); ACIS soft (0.5-1.2keV) energy
band (fluxbbaper90hilims)
2819-2826 E8.3 mW/m2 FBB90u ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV]; ACIS ultrasoft (0.2-0.5keV)
energy band (fluxbbaper90_u)
2828-2835 E8.3 mW/m2 b_FBB90u ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); ACIS ultrasoft (0.2-0.5keV)
energy band (fluxbbaper90lolimu)
2837-2844 E8.3 mW/m2 B_FBB90u ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); ACIS ultrasoft (0.2-0.5keV)
energy band (fluxbbaper90hilimu)
2846-2853 E8.3 mW/m2 FBB90w ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV]; HRC wide (∼0.1-10.0keV)
energy band (fluxbbaper90_w)
2855-2862 E8.3 mW/m2 b_FBB90w ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% lower confidence
limit); HRC wide (∼0.1-10.0keV) energy
band (fluxbbaper90lolimw)
2864-2871 E8.3 mW/m2 B_FBB90w ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
black body model [NH=NH(Gal);
kT=0.75keV] (68% upper confidence
limit); HRC wide (∼0.1-10.0keV) energy
band (fluxbbaper90hilimw)
2873-2880 E8.3 mW/m2 FBS90b ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV]; ACIS broad (0.5-7.0keV)
energy band (fluxbremsaper90_b)
2882-2889 E8.3 mW/m2 b_FBS90b ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% lower confidence limit);
ACIS broad (0.5-7.0keV) energy band
(fluxbremsaper90lolimb)
2891-2898 E8.3 mW/m2 B_FBS90b ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% upper confidence limit);
ACIS broad (0.5-7.0keV) energy band
(fluxbremsaper90hilimb)
2900-2907 E8.3 mW/m2 FBS90h ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV]; ACIS hard (2.0-7.0keV)
energy band (fluxbremsaper90_h)
2909-2916 E8.3 mW/m2 b_FBS90h ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% lower confidence limit);
ACIS hard (2.0-7.0keV) energy band
(fluxbremsaper90lolimh)
2918-2925 E8.3 mW/m2 B_FBS90h ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% upper confidence limit);
ACIS hard (2.0-7.0keV) energy band
(fluxbremsaper90hilimh)
2927-2934 E8.3 mW/m2 FBS90m ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV]; ACIS medium (1.2-2.0keV)
energy band (fluxbremsaper90_m)
2936-2943 E8.3 mW/m2 b_FBS90m ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% lower confidence limit);
ACIS medium (1.2-2.0keV) energy band
(fluxbremsaper90lolimm)
2945-2952 E8.3 mW/m2 B_FBS90m ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% upper confidence limit);
ACIS medium (1.2-2.0keV) energy band
(fluxbremsaper90hilimm)
2954-2961 E8.3 mW/m2 FBS90s ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV]; ACIS soft (0.5-1.2keV)
energy band (fluxbremsaper90_s)
2963-2970 E8.3 mW/m2 b_FBS90s ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% lower confidence limit);
ACIS soft (0.5-1.2keV) energy band
(fluxbremsaper90lolims)
2972-2979 E8.3 mW/m2 B_FBS90s ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% upper confidence limit);
ACIS soft (0.5-1.2keV) energy band
(fluxbremsaper90hilims)
2981-2988 E8.3 mW/m2 FBS90u ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV]; ACIS ultrasoft (0.2-0.5keV)
energy band (fluxbremsaper90_u)
2990-2997 E8.3 mW/m2 b_FBS90u ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% lower confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxbremsaper90lolimu)
2999-3006 E8.3 mW/m2 B_FBS90u ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% upper confidence limit);
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxbremsaper90hilimu)
3008-3015 E8.3 mW/m2 FBS90w ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV]; HRC wide (∼0.1-10.0keV)
energy band (fluxbremsaper90_w)
3017-3024 E8.3 mW/m2 b_FBS90w ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% lower confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxbremsaper90lolimw)
3026-3033 E8.3 mW/m2 B_FBS90w ? PSF90% ECF aperture model energy flux
inferred from the canonical absorbed
bremsstrahlung model [NH=NH(Gal);
kT=3.5keV] (68% upper confidence limit);
HRC wide (∼0.1-10.0keV) energy band
(fluxbremsaper90hilimw)
3035-3042 E8.3 mW/m2 FAP90b ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV];
ACIS broad (0.5-7.0keV) energy band
(fluxapecaper90_b)
3044-3051 E8.3 mW/m2 b_FAP90b ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% lower confidence limit); ACIS broad
(0.5-7.0keV) energy band
(fluxapecaper90lolimb)
3053-3060 E8.3 mW/m2 B_FAP90b ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% upper confidence limit); ACIS broad
(0.5-7.0keV) energy band
(fluxapecaper90hilimb)
3062-3069 E8.3 mW/m2 FAP90h ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV];
ACIS hard (2.0-7.0keV) energy band
(fluxapecaper90_h)
3071-3078 E8.3 mW/m2 b_FAP90h ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% lower confidence limit); ACIS hard
(2.0-7.0keV) energy band
(fluxapecaper90lolimh)
3080-3087 E8.3 mW/m2 B_FAP90h ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% upper confidence limit); ACIS hard
(2.0-7.0keV) energy band
(fluxapecaper90hilimh)
3089-3096 E8.3 mW/m2 FAP90m ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV];
ACIS medium (1.2-2.0keV) energy band
(fluxapecaper90_m)
3098-3105 E8.3 mW/m2 b_FAP90m ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% lower confidence limit); ACIS
medium (1.2-2.0keV) energy band
(fluxapecaper90lolimm)
3107-3114 E8.3 mW/m2 B_FAP90m ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% upper confidence limit); ACIS
medium (1.2-2.0keV) energy band
(fluxapecaper90hilimm)
3116-3123 E8.3 mW/m2 FAP90s ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV];
ACIS soft (0.5-1.2keV) energy band
(fluxapecaper90_s)
3125-3132 E8.3 mW/m2 b_FAP90s ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% lower confidence limit); ACIS soft
(0.5-1.2keV) energy band
(fluxapecaper90lolims)
3134-3141 E8.3 mW/m2 B_FAP90s ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% upper confidence limit); ACIS soft
(0.5-1.2keV) energy band
(fluxapecaper90hilims)
3143-3150 E8.3 mW/m2 FAP90u ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV];
ACIS ultrasoft (0.2-0.5keV) energy band
(fluxapecaper90_u)
3152-3159 E8.3 mW/m2 b_FAP90u ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% lower confidence limit); ACIS
ultrasoft (0.2-0.5keV) energy band
(fluxapecaper90lolimu)
3161-3168 E8.3 mW/m2 B_FAP90u ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% upper confidence limit); ACIS
ultrasoft (0.2-0.5keV) energy band
(fluxapecaper90hilimu)
3170-3177 E8.3 mW/m2 FAP90w ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV];
HRC wide (∼0.1-10.0keV) energy band
(fluxapecaper90_w)
3179-3186 E8.3 mW/m2 b_FAP90w ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% lower confidence limit); HRC wide
(∼0.1-10.0keV) energy band
(fluxapecaper90lolimw)
3188-3195 E8.3 mW/m2 B_FAP90w ? PSF 90% ECF aperture model energy flux
inferred from the canonical absorbed
APEC model [NH=NH(Gal); kT=6.5keV]
(68% upper confidence limit); HRC wide
(∼0.1-10.0keV) energy band
(fluxapecaper90hilimw)
3197-3202 F6.2 10+20cm-2 NHGal ? Galactic N_H column density in
direction of source (nh_gal)
3204-3210 F7.4 --- HRhm ? ACIS hard (2.0-7.0keV) - medium
(1.2-2.0keV) energy band photon flux
hardness ratio (hard_hm)
3212-3218 F7.4 --- b_HRhm ? ACIS hard (2.0-7.0keV) - medium
(1.2-2.0keV) energy band photon flux
hardness ratio (68% lower confidence
limit) (hardhmlolim)
3220-3226 F7.4 --- B_HRhm ? ACIS hard (2.0-7.0keV) - medium
(1.2-2.0keV) energy band photon flux
hardness ratio (68% upper confidence
limit) (hardhmhilim)
3228-3232 F5.3 --- ViPhm ? Inter-observation ACIS hard
(2.0-7.0keV) - medium (1.2-2.0keV)
energy band photon flux hardness ratio
variability probability
(varinterhardprobhm)
3234-3242 E9.7 --- ViShm ? Inter-observation ACIS hard
(2.0-7.0keV) - medium (1.2-2.0keV)
energy band photon flux hardness ratio
variability standard deviation
(varinterhardsigmahm)
3244-3250 F7.4 --- HRhs ? ACIS hard (2.0-7.0keV) - soft
(0.5-1.2keV) energy band photon flux
hardness ratio (hard_hs)
3252-3258 F7.4 --- b_HRhs ? ACIS hard (2.0-7.0keV) - soft
(0.5-1.2keV) energy band photon flux
hardness ratio (68% lower confidence
limit) (hardhslolim)
3260-3266 F7.4 --- B_HRhs ? ACIS hard (2.0-7.0keV) - soft
(0.5-1.2keV) energy band photon flux
hardness ratio (68% upper confidence
limit) (hardhshilim)
3268-3272 F5.3 --- ViPhs ? Inter-observation ACIS hard
(2.0-7.0keV) - soft (0.5-1.2keV) energy
band photon flux hardness ratio
variability probability
(varinterhardprobhs)
3274-3282 E9.7 --- ViShs ? Inter-observation ACIS hard
(2.0-7.0keV) - soft (0.5-1.2keV) energy
band photon flux hardness ratio
variability standard deviation
(varinterhardsigmahs)
3284-3290 F7.4 --- HRms ? ACIS medium (1.2-2.0keV) - soft
(0.5-1.2keV) energy band photon flux
hardness ratio (hard_ms)
3292-3298 F7.4 --- b_HRms ? ACIS medium (1.2-2.0keV) - soft
(0.5-1.2keV) energy band photon flux
hardness ratio (68% lower confidence
limit) (hardmslolim)
3300-3306 F7.4 --- B_HRms ? ACIS medium (1.2-2.0keV) - soft
(0.5-1.2keV) energy band photon flux
hardness ratio (68% upper confidence
limit) (hardmshilim)
3308-3312 F5.3 --- ViPms ? Inter-observation ACIS medium
(1.2-2.0keV) - soft (0.5-1.2keV) energy
band photon flux hardness ratio
variability probability
(varinterhardprobms)
3314-3322 E9.7 --- ViSms ? Inter-observation ACIS medium
(1.2-2.0keV) - soft (0.5-1.2keV) energy
band photon flux hardness ratio
variability standard deviation
(varinterhardsigmams)
3324-3331 E8.3 mW/m2 FPL0.5-7 ? Net integrated 0.5-7.0 keV energy flux
of the best fitting absorbed power-law
model spectrum to the source region
aperture PI spectrum (flux_powlaw)
3333-3340 E8.3 mW/m2 b_FPL0.5-7 ? Net 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) (fluxpowlawlolim)
3342-3349 E8.3 mW/m2 B_FPL0.5-7 ? Net 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) (fluxpowlawhilim)
3351-3356 F6.3 --- GamPL ? Photon index, defined as
FE∼E(-Gamma), of the best fitting
absorbed power-law model spectrum to the
source region aperture PI spectrum
(powlaw_gamma)
3358-3364 F7.3 --- b_GamPL ? Photon index, defined as
FE∼E(-Gamma), of the best fitting
absorbed power-law model spectrum to the
source region aperture PI spectrum (68%
lower confidence limit)
(powlawgammalolim)
3366-3372 F7.3 --- B_GamPL ? Photon index, defined as
FE∼E(-Gamma), of the best fitting
absorbed power-law model spectrum to the
source region aperture PI spectrum (68%
upper confidence limit)
(powlawgammahilim)
3374-3382 E9.7 10+20cm-2 NHPL ? N_H column density of the best fitting
absorbed power-law model spectrum to the
source region aperture PI spectrum
(powlaw_nh)
3384-3393 F10.5 10+20cm-2 b_NHPL ? N_H column density of the best fitting
absorbed power-law model spectrum to the
source region aperture PI spectrum (68%
lower confidence limit)
(powlawnhlolim)
3395-3403 E9.7 10+20cm-2 B_NHPL ? N_H column density of the best fitting
absorbed power-law model spectrum to the
source region aperture PI spectrum (68%
upper confidence limit)
(powlawnhhilim)
3405-3413 E9.7 --- AmpPL ? Amplitude of the best fitting absorbed
power-law model spectrum to the source
region aperture PI spectrum
(powlaw_ampl)
3415-3423 E9.7 --- b_AmpPL ? Amplitude of the best fitting absorbed
power-law model spectrum to the source
region aperture PI spectrum (68% lower
confidence limit) (powlawampllolim)
3425-3433 E9.7 --- B_AmpPL ? Amplitude of the best fitting absorbed
power-law model spectrum to the source
region aperture PI spectrum (68% upper
confidence limit) (powlawamplhilim)
3435-3440 F6.3 --- Chi2PL ? chi-square statistic per degree of
freedom of the best fitting absorbed
power-law model spectrum to the source
region aperture PI spectrum
(powlaw_stat)
3442-3449 E8.3 mW/m2 FBB0.5-7 ? Net integrated 0.5-7.0 keV energy flux
of the best fitting absorbed black body
model spectrum to the source region
aperture PI spectrum (flux_bb)
3451-3458 E8.3 mW/m2 b_FBB0.5-7 ? Net 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) (fluxbblolim)
3460-3467 E8.3 mW/m2 B_FBB0.5-7 ? Net 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) (fluxbbhilim)
3469-3476 F8.4 keV kTBB ? Temperature (kT) of the best fitting
absorbed black body model spectrum to
the source region aperture PI spectrum
(bb_kt)
3478-3485 F8.5 keV b_kTBB ? Temperature (kT) of the best fitting
absorbed black body model spectrum to
the source region aperture PI spectrum
(68% lower confidence limit)
(bbktlolim)
3487-3495 E9.4 keV B_kTBB ? Temperature (kT) of the best fitting
absorbed black body model spectrum to
the source region aperture PI spectrum
(68% upper confidence limit)
(bbkthilim)
3497-3505 E9.7 10+20cm-2 NHBB ? N_H column density of the best fitting
absorbed black body model spectrum to
the source region aperture PI spectrum
(bb_nh)
3507-3516 F10.5 10+20cm-2 b_NHBB ? N_H column density of the best fitting
absorbed black body model spectrum to
the source region aperture PI spectrum
(68% lower confidence limit)
(bbnhlolim)
3518-3526 E9.6 10+20cm-2 B_NHBB ? N_H column density of the best fitting
absorbed black body model spectrum to
the source region aperture PI spectrum
(68% upper confidence limit)
(bbnhhilim)
3528-3536 E9.7 --- AmpBB ? Amplitude of the best fitting absorbed
black body model spectrum to the source
region aperture PI spectrum (bb_ampl)
3538-3546 E9.7 --- b_AmpBB ? Amplitude of the best fitting absorbed
black body model spectrum to the source
region aperture PI spectrum (68% lower
confidence limit) (bbampllolim)
3548-3556 E9.7 --- B_AmpBB ? Amplitude of the best fitting absorbed
black body model spectrum to the source
region aperture PI spectrum (68% upper
confidence limit) (bbamplhilim)
3558-3564 F7.3 --- Chi2BB ? chi-square statistic per degree of
freedom of the best fitting absorbed
black body model spectrum to the source
region aperture PI spectrum (bb_stat)
3566-3573 E8.3 mW/m2 FBS0.5-7 ? Net integrated 0.5-7.0 keV energy flux
of the best fitting absorbed
bremsstrahlung model spectrum to the
source region aperture PI spectrum
(flux_brems)
3575-3582 E8.3 mW/m2 b_FBS0.5-7 ? Net 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)
(fluxbremslolim)
3584-3591 E8.3 mW/m2 B_FBS0.5-7 ? Net 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)
(fluxbremshilim)
3593-3603 F11.7 keV kTBS ? Temperature (kT) of the best fitting
absorbed bremsstrahlung model spectrum
to the source region aperture PI
spectrum (brems_kt)
3605-3612 F8.5 keV b_kTBS ? Temperature (kT) of the best fitting
absorbed bremsstrahlung model spectrum
to the source region aperture PI
spectrum (68% lower confidence limit)
(bremsktlolim)
3614-3622 E9.5 keV B_kTBS ? Temperature (kT) of the best fitting
absorbed bremsstrahlung model spectrum
to the source region aperture PI
spectrum (68% upper confidence limit)
(bremskthilim)
3624-3632 E9.7 10+20cm-2 NHBS ? N_H column density of the best fitting
absorbed bremsstrahlung model spectrum
to the source region aperture PI
spectrum (brems_nh)
3634-3642 E9.5 10+20cm-2 b_NHBS ? N_H column density of the best fitting
absorbed bremsstrahlung model spectrum
to the source region aperture PI
spectrum (68% lower confidence limit)
(bremsnhlolim)
3644-3652 E9.5 10+20cm-2 B_NHBS ? N_H column density of the best fitting
absorbed bremsstrahlung model spectrum
to the source region aperture PI
spectrum (68% upper confidence limit)
(bremsnhhilim)
3654-3662 E9.7 --- AmpBS ? Amplitude of the best fitting absorbed
bremsstrahlung model spectrum to the
source region aperture PI spectrum
(brems_norm)
3664-3672 E9.7 --- b_AmpBS ? Amplitude of the best fitting absorbed
bremsstrahlung model spectrum to the
source region aperture PI spectrum (68%
lower confidence limit)
(bremsnormlolim)
3674-3682 E9.7 --- B_AmpBS ? Amplitude of the best fitting absorbed
bremsstrahlung model spectrum to the
source region aperture PI spectrum (68%
upper confidence limit)
(bremsnormhilim)
3684-3689 F6.3 --- Chi2BS ? chi-square statistic per degree of
freedom of the best fitting absorbed
bremsstrahlung model spectrum to the
source region aperture PI spectrum
(brems_stat)
3691-3698 E8.3 mW/m2 FA0.5-7.0 ? Net integrated 0.5-7.0 keV energy flux
of the best fitting absorbed APEC model
spectrum to the source region aperture
PI spectrum (flux_apec)
3700-3707 E8.3 mW/m2 b_FA0.5-7.0 ? Net 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)
(fluxapeclolim)
3709-3716 E8.3 mW/m2 B_FA0.5-7.0 ? Net 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)
(fluxapechilim)
3718-3725 F8.5 keV kTA ? Temperature (kT) of the best fitting
absorbed APEC model spectrum to the
source region aperture PI spectrum
(apec_kt)
3727-3735 F9.6 keV b_kTA ? Temperature (kT) of the best fitting
absorbed APEC model spectrum to the
source region aperture PI spectrum
(68% lower confidence limit)
(apecktlolim)
3737-3744 F8.4 keV B_kTA ? Temperature (kT) of the best fitting
absorbed APEC model spectrum to the
source region aperture PI spectrum
(68% upper confidence limit)
(apeckthilim)
3746-3754 E9.7 --- Abund ? Abundance of the best fitting absorbed
APEC model spectrum to the source
region aperture PI spectrum (apec_abund)
3756-3764 F9.7 --- b_Abund ? Abundance of the best fitting absorbed
APEC model spectrum to the source region
aperture PI spectrum
(68% lower confidence limit)
(apecabundlolim)
3766-3774 E9.6 --- B_Abund ? Abundance of the best fitting absorbed
APEC model spectrum to the source region
aperture PI spectrum (68% upper
confidence limit) (apecabundhilim)
3776-3785 E10.7 --- z ? Redshift of the best fitting absorbed
APEC model spectrum to the source region
aperture PI spectrum (apec_z)
3787-3796 E10.7 --- b_z ? Redshift of the best fitting absorbed
APEC model spectrum to the source region
aperture PI spectrum (68% lower
confidence limit) (apeczlolim)
3798-3808 F11.7 --- B_z ? Redshift of the best fitting absorbed
APEC model spectrum to the source region
aperture PI spectrum (68% upper
confidence limit) (apeczhilim)
3810-3818 E9.7 10+20cm-2 NH ? N_H column density of the best fitting
absorbed APEC model spectrum to the
source region aperture PI spectrum
(apec_nh)
3820-3830 F11.6 10+20cm-2 b_NH ? N_H column density of the best fitting
absorbed APEC model spectrum to the
source region aperture PI spectrum (68%
lower confidence limit) (apecnhlolim)
3832-3840 E9.5 10+20cm-2 B_NH ? N_H column density of the best fitting
absorbed APEC model spectrum to the
source region aperture PI spectrum (68%
upper confidence limit) (apecnhhilim)
3842-3850 E9.7 --- Amp ? Amplitude of the best fitting absorbed
APEC model spectrum to the source region
aperture PI spectrum (apec_norm)
3852-3860 E9.7 --- b_Amp ? Amplitude of the best fitting absorbed
APEC model spectrum to the source region
aperture PI spectrum (68% lower
confidence limit) (apecnormlolim)
3862-3870 E9.7 --- B_Amp ? Amplitude of the best fitting absorbed
APEC model spectrum to the source region
aperture PI spectrum (68% upper
confidence limit) (apecnormhilim)
3872-3877 F6.3 --- Chi2 ? chi-square statistic per degree of
freedom of the best fitting absorbed
APEC model spectrum to the source region
aperture PI spectrum (apec_stat)
3879-3880 I2 --- VaGLIb ? Intra-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 (0.5-7.0keV)
energy band (varintraindex_b)
3882-3886 F5.3 --- Vab ? Intra-observation Gregory-Loredo
variability probability (highest value
across all observations); ACIS broad
(0.5-7.0keV) energy band
(varintraprob_b)
3888-3892 F5.3 --- VaKSb ? Intra-observation Kolmogorov-Smirnov
test variability probability (highest
value across all observations); ACIS
broad (0.5-7.0keV) energy band
(ksintraprob_b)
3894-3898 F5.3 --- VaKPb ? Intra-observation Kuiper's test
variability probability (highest value
across all observations); ACIS broad
(0.5-7.0keV) energy band
(kpintraprob_b)
3900-3901 I2 --- VaGLIh ? Intra-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 (2.0-7.0keV)
energy band (varintraindex_h)
3903-3907 F5.3 --- Vah ? Intra-observation Gregory-Loredo
variability probability (highest value
across all observations); ACIS hard
(2.0-7.0keV) energy band
(varintraprob_h)
3909-3913 F5.3 --- VaKSh ? Intra-observation Kolmogorov-Smirnov
test variability probability (highest
value across all observations); ACIS
hard (2.0-7.0keV) energy band
(ksintraprob_h)
3915-3919 F5.3 --- VaKPh ? Intra-observation Kuiper's test
variability probability (highest value
across all observations); ACIS hard
(2.0-7.0keV) energy band
(kpintraprob_h)
3921-3922 I2 --- VaGLIm ? Intra-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 (1.2-2.0keV)
energy band (varintraindex_m)
3924-3928 F5.3 --- Vam ? Intra-observation Gregory-Loredo
variability probability (highest value
across all observations); ACIS medium
(1.2-2.0keV) energy band
(varintraprob_m)
3930-3934 F5.3 --- VaKSm ? Intra-observation Kolmogorov-Smirnov
test variability probability (highest
value across all observations); ACIS
medium (1.2-2.0keV) energy band
(ksintraprob_m)
3936-3940 F5.3 --- VaKPm ? Intra-observation Kuiper's test
variability probability (highest value
across all observations); ACIS medium
(1.2-2.0keV) energy band
(kpintraprob_m)
3942-3943 I2 --- VaGLIs ? Intra-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 (0.5-1.2keV)
energy band (varintraindex_s)
3945-3949 F5.3 --- Vas ? Intra-observation Gregory-Loredo
variability probability (highest value
across all observations); ACIS soft
(0.5-1.2keV) energy band
(varintraprob_s)
3951-3955 F5.3 --- VaKSs ? Intra-observation Kolmogorov-Smirnov
test variability probability (highest
value across all observations); ACIS
soft (0.5-1.2keV) energy band
(ksintraprob_s)
3957-3961 F5.3 --- VaKPs ? Intra-observation Kuiper's test
variability probability (highest value
across all observations); ACIS soft
(0.5-1.2keV) energy band
(kpintraprob_s)
3963-3964 I2 --- VaGLIu ? Intra-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
(0.2-0.5keV) energy band
(varintraindex_u)
3966-3970 F5.3 --- Vau ? Intra-observation Gregory-Loredo
variability probability (highest value
across all observations); ACIS ultrasoft
(0.2-0.5keV) energy band
(varintraprob_u)
3972-3976 F5.3 --- VaKSu ? Intra-observation Kolmogorov-Smirnov
test variability probability (highest
value across all observations); ACIS
ultrasoft (0.2-0.5keV) energy band
(ksintraprob_u)
3978-3982 F5.3 --- VaKPu ? Intra-observation Kuiper's test
variability probability (highest value
across all observations); ACIS
ultrasoft (0.2-0.5keV) energy band
(kpintraprob_u)
3984-3985 I2 --- VaGLIw ? Intra-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 (∼0.1-10.0keV)
energy band (varintraindex_w)
3987-3991 F5.3 --- Vaw ? Intra-observation Gregory-Loredo
variability probability (highest value
across all observations); HRC wide
(∼0.1-10.0keV) energy band
(varintraprob_w)
3993-3997 F5.3 --- VaKSw ? Intra-observation Kolmogorov-Smirnov
test variability probability (highest
value across all observations); HRC wide
(∼0.1-10.0keV) energy band
(ksintraprob_w)
3999-4003 F5.3 --- VaKPw ? Intra-observation Kuiper's test
variability probability (highest value
across all observations); HRC wide
(∼0.1-10.0keV) energy band
(kpintraprob_w)
4005 I1 --- ViIb ? Inter-observation variability index in
the range [0, 10]: indicates whether the
source region photon flux is constant
between observations; ACIS broad
(0.5-7.0keV) energy band
(varinterindex_b)
4007-4011 F5.3 --- Vib ? Inter-observation variability
probability, calculated from the chi2
distribution of the photon fluxes of the
individual observations; ACIS broad
(0.5-7.0keV) energy band
(varinterprob_b)
4013-4021 E9.7 ph/s/cm+2 ViSb ? Inter-observation flux variability
standard deviation; the spread of the
individual observation photon fluxes
about the error weighted mean; ACIS
broad (0.5-7.0keV) energy band
(varintersigma_b)
4023 I1 --- ViIh ? Inter-observation variability index in
the range [0, 10]: indicates whether the
source region photon flux is constant
between observations; ACIS hard
(2.0-7.0keV) energy band
(varinterindex_h)
4025-4029 F5.3 --- Vih ? Inter-observation variability
probability, calculated from the chi2
distribution of the photon fluxes of the
individual observations; ACIS hard
(2.0-7.0keV) energy band
(varinterprob_h)
4031-4039 E9.7 ph/s/cm+2 ViSh ? Inter-observation flux variability
standard deviation; the spread of the
individual observation photon fluxes
about the error weighted mean; ACIS hard
(2.0-7.0keV) energy band
(varintersigma_h)
4041 I1 --- ViIm ? Inter-observation variability index in
the range [0, 10]: indicates whether the
source region photon flux is constant
between observations; ACIS medium
(1.2-2.0keV) energy band
(varinterindex_m)
4043-4047 F5.3 --- Vim ? Inter-observation variability
probability, calculated from the chi2
distribution of the photon fluxes of the
individual observations; ACIS medium
(1.2-2.0keV) energy band
(varinterprob_m)
4049-4057 E9.7 ph/s/cm+2 ViSm ? Inter-observation flux variability
standard deviation; the spread of the
individual observation photon fluxes
about the error weighted mean; ACIS
medium (1.2-2.0keV) energy band
(varintersigma_m)
4059 I1 --- ViIs ? Inter-observation variability index in
the range [0, 10]: indicates whether the
source region photon flux is constant
between observations; ACIS soft
(0.5-1.2keV) energy band
(varinterindex_s)
4061-4065 F5.3 --- Vis ? Inter-observation variability
probability, calculated from the chi2
distribution of the photon fluxes of the
individual observations; ACIS soft
(0.5-1.2keV) energy band
(varinterprob_s)
4067-4075 E9.7 ph/s/cm+2 ViSs ? Inter-observation flux variability
standard deviation; the spread of the
individual observation photon fluxes
about the error weighted mean; ACIS soft
(0.5-1.2keV) energy band
(varintersigma_s)
4077 I1 --- ViIu ? Inter-observation variability index in
the range [0, 10]: indicates whether the
source region photon flux is constant
between observations; ACIS ultrasoft
(0.2-0.5keV) energy band
(varinterindex_u)
4079-4083 F5.3 --- Viu ? Inter-observation variability
probability, calculated from the chi2
distribution of the photon fluxes of the
individual observations; ACIS ultrasoft
(0.2-0.5keV) energy band
(varinterprob_u)
4085-4093 E9.7 ph/s/cm+2 ViSu ? Inter-observation flux variability
standard deviation; the spread of the
individual observation photon fluxes
about the error weighted mean;
ACIS ultrasoft (0.2-0.5keV) energy band
(varintersigma_u)
4095 I1 --- ViIw ? Inter-observation variability index in
the range [0, 10]: indicates whether the
source region photon flux is constant
between observations; HRC wide
(∼0.1-10.0keV) energy band
(varinterindex_w)
4097-4101 F5.3 --- Viw ? Inter-observation variability
probability, calculated from the chi2
distribution of the photon fluxes of the
individual observations; HRC wide
(∼0.1-10.0keV) energy band
(varinterprob_w)
4103-4111 E9.7 ph/s/cm+2 ViSw ? Inter-observation flux variability
standard deviation; the spread of the
individual observation photon fluxes
about the error weighted mean; HRC wide
(∼0.1-10.0keV) energy band
(varintersigma_w)
4113-4115 I3 --- Nac ? Total number of ACIS imaging
observations contributing to the Master
Sources Table record of the source
(acis_num)
4117 I1 --- Nac/hetg ? Total number of ACIS/HETG observations
contributing to the Master Sources Table
record of the source (acishetgnum)
4119 I1 --- Nac/letg ? Total number of ACIS/LETG observations
contributing to the Master Sources Table
record of the source (acisletgnum)
4121-4123 I3 --- Nhrc ? Total number of HRC imaging
observations contributing to the Master
Sources Table record of the source
(hrc_num)
4125 I1 --- Nhrc/h ? Total number of HRC/HETG observations
contributing to the Master Sources Table
record of the source (hrchetgnum)
4127 I1 --- Nhrc/l ? Total number of HRC/LETG observations
contributing to the Master Sources Table
record of the source (hrcletgnum)
4129-4137 F9.1 s TimeA ? Total livetime for all ACIS imaging
observations contributing to the
Master Sources Table record of the
source (Tacis_time)
4139-4147 F9.1 s TimeH ? Total livetime for all HRC imaging
observations contributing to the Master
Sources Table record of the source
(Thrc_time)
--------------------------------------------------------------------------------
Note (1): 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.
Note (2): averaged over all contributing observations, and calculated by
counting X-ray events.
--------------------------------------------------------------------------------
History:
From doi:10.25574/csc2
(End) Patricia Vannier [CDS] 10-Dec-2024