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CSC - Chandra Source Catalog, v2.0 |
HEASARC Archive |
Overview
The Chandra Source Catalog (CSC) is the definitive catalog of X-ray sources detected by the Chandra X-ray Observatory. By combining Chandra's sub-arcsecond on-axis spatial resolution and low instrumental background with consistent data processing, the CSC delivers a wide variety of uniformly calibrated properties and science ready data products for detected sources over four decades of flux. The second major release of the catalog, CSC 2.0, includes measured properties for 317,167 unique compact and extended X-ray sources in the sky, allowing statistical analysis of large samples, as well as individual source studies in the "Master Sources" table, provided herein.The extracted properties are provided for 928,280 individual observation detections, identified in 10,382 Chandra ACIS and HRC-I imaging observations released publicly through the end of 2014, at the Chandra X-ray Center. CSC 2.0 includes -- as an "alpha" release -- photometric properties for 1,299 highly extended (> ~30") sources, together with surface brightness polygons for several contour levels.
The sensitivity limit for compact sources in CSC 2.0 is ~5 net counts (a factor of >~2 better than the previous catalog release). This improvement is achieved by using a two-stage approach that involves co-adding multiple observations of the same field prior to source detection, and then using an optimized source detection method.
For each X-ray detection and source, the catalog provides a detailed set of more than 100 tabulated positional, spatial, photometric, spectral, and temporal properties (each with associated lower and upper confidence intervals and measured in multiple energy bands). The catalog Bayesian aperture photometry code produces robust photometric probability density functions (PDFs), even in crowded fields and for low count detections. Release 2 uses a Bayesian Blocks analysis to identify multiple observations of the same source that have similar photometric properties, and these are analyzed simultaneously to improve S/N.
The energy bands used to derive many of the CSC properties are defined in Table 4 of the reference paper: ultrasoft (u: 0.2-0.5 keV), soft (s: 0.5-1.2 keV), medium (m: 1.2-2.0 keV), hard (h: 2.0-7.0) and broad (b: 0.5-7.0 keV) for the ACIS energy bands, and wide (w: 0.1-10.0 keV) for the HRC energy band. The energy bands are chosen to optimize the detectability of X-ray sources while simultaneously maximizing the discrimination between different spectral shapes on X-ray color-color diagrams.
Numerous source-specific catalog properties are evaluated within defined apertures. The authors define the "PSF 90% ECF aperture" for each source to be the ellipse that encloses 90% of the total counts in a model PSF centered on the source position. Because the size of the PSF is energy-dependent, the dimensions of the PSF 90% ECF aperture vary with energy band. They define the "source region aperture" for each source to be equal to the corresponding 3-sigma source region ellipse included in the merged source list, scaled by a factor of 1.5. Like the PSF 90% ECF aperture, the source region aperture is also centered on the source position, but the dimensions of the aperture are independent of energy band.
Catalog Bibcode
2010ApJS..189...37EReferences
The Chandra Source Catalog
Evans I.N., Primini F.A., Glotfelty C.S., Anderson C.S., Bonaventura N.R.,
Chen J.C., Davis J.E., Doe S.M., Evans J.D., Fabbiano G., Galle E.C.,
Gibbs D.G., Grier J.D., Hain R.M., Hall D.M., Harbo P.N., He X.,
Houck J.C., Karovska M., Kashyap V.L., Lauer J., McCollough M.L.,
McDowell J.C., Miller J.B., Mitschang A.W., Morgan D.L., Mossman A.E.,
Nichols J.S., Nowak M.A., Plummer D.A., Refsdal B.L., Rots A.H.,
Siemiginowska A., Sundheim B.A., Tibbetts M.S., Van Stone D.W.,
Winkelman S.L., Zografou P.
<Astrophys. J. Suppl. Ser. 189, 37 (2010)>
=2010ApJS..189...37E
Provenance
This database table was ingested by the HEASARC in November 2019 and is based on a download of the online version of the Chandra Source Catalog, v2.0, at the CXC using the CLI. Refer to http://cxc.harvard.edu/csc/ for details.Parameters
Name
The Chandra Source Catalog name in the IAU position-based nomenclature, viz.,
'2CXO Jhhmmss.s{+,-}ddmmss', where the 'CXO' stands for Chandra X-ray
Observatory and the '2' stands for version 2 of this catalog.
RA
The Right Ascension of the X-ray source in the selected equinox. This was
given in ICRS coordinates in the original source table and was determined by
statistically averaging the positions of detections from the individual
stacked observations that are uniquely matched to the source. The calculation
of the averaged positions and position uncertainties is described in detail
in the How and Why topic 'Source Position Errors in the Master Sources Table'
at https://cxc.harvard.edu/csc/why/err_ellipse_msc.html.
Dec
The Declination of the X-ray source in the selected equinox. This was given
in ICRS coordinates in the original source table and was determined by
statistically averaging the positions of detections from the individual
stacked observations that are uniquely matched to the source. The calculation
of the averaged positions and position uncertainties is described in detail
in the How and Why topic 'Source Position Errors in the Master Sources Table'
at https://cxc.harvard.edu/csc/why/err_ellipse_msc.html.
LII
The Galactic Longitude (equinox J2000.0, epoch J2000.0) of the X-ray source.
BII
The Galactic Latitude (equinox J2000.0, epoch J2000.0) of the X-ray source.
Error_Ellipse_R0
The major radius of the 95% confidence level position error ellipse, in
arcseconds. The source position error ellipses in the Master Sources Table
include a component to account for the absolute uncertainty in the astrometry
relative to the ICRS reference frame. This uncertainty, 0.71 arcsec (95%
confidence) in each axis, is derived from comparisons of source positions
from release 2.0 detections relative to the Sloan Digital Sky Survey, and is
added in quadrature to the statistically averaged position uncertainties from
the stacked observation detections.
Error_Ellipse_R1
The minor radius of the 95% confidence level position error ellipse, in
arcseconds. The source position error ellipses in the Master Sources Table
include a component to account for the absolute uncertainty in the astrometry
relative to the ICRS reference frame. This uncertainty, 0.71 arcsec (95%
confidence) in each axis, is derived from comparisons of source positions
from release 2.0 detections relative to the Sloan Digital Sky Survey, and is
added in quadrature to the statistically averaged position uncertainties from
the stacked observation detections.
Error_Ellipse_Angle
The position angle (ref. local true north) of the major axis of the 95%
confidence level error ellipse, in degrees.
Extent_Flag
This is set to 'T' if the source is extended or the deconvolved source extent
is inconsistent with a point source at the 90% confidence level in one or
more observations and energy bands.
Conf_Flag
This is set to 'T' if the source may be confused (source and/or background
regions overlap in one or more contributing stacked observations). For an
extended source, this flag is NULL.
Pileup_Flag
This is set to 'T' if the ACIS pile-up fraction exceeds ~ 10% in all
observations; source properties may be affected. For an extended source, this
flag is NULL.
Var_Flag
This is set to 'T' if the source displays flux variability within one or more
observations, or between observations, in one or more energy bands. For an
extended source, this flag is NULL.
Streak_Src_Flag
This is set to 'T' if the source is located on an ACIS readout streak in all
observations for compact sources or in any observations for extended sources;
source properties may be affected.
Sat_Src_Flag
This is set to 'T' if the source has significant pile-up in all observations;
source properties are unreliable. For extended sources, this flag is NULL.
Man_Add_Flag
This is set to 'T' if the source was manually added in the catalog via human
review.
Man_Inc_Flag
This is set to 'T' if the source was manually included in the catalog via
human review (detection was rejected by automated criteria).
Man_Reg_Flag
This is set to 'T' if the source region parameters (dimensions, initial guess
position input to the Maximum Likelihood Estimator fit) were manually
modified via human review.
Man_Match_Flag
This is set to 'T' if the source detections were manually matched between
overlapping stacked observations via human review, i.e. the observation
detections were not matched, or were matched incorrectly, by the detection
matching algorithm.
Man_Pos_Flag
This is set to 'T' if the best fit source position was manually modified via
human review.
Var_Inter_Hard_Flag
This is set to 'T' if the source hardness ratios are statistically
inconsistent between two or more observations. For an extended object, this
flag is NULL.
B_Major_Axis
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent; ACIS broad (0.5-7.0 keV) energy band.
H_Major_Axis
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent; ACIS hard (2.0-7.0 keV) energy band.
M_Major_Axis
The 1-sigma radius(in arcsec) along the major axis of the ellipse defining
the deconvolved source extent; ACIS medium (1.2-2.0 keV) energy band.
S_Major_Axis
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent; ACIS soft (0.5-1.2 keV) energy band.
U_Major_Axis
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent; ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Major_Axis
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent; HRC wide (~0.1-10.0 keV) energy band.
B_Major_Axis_Lo
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent (68% lower confidence limit); ACIS broad
(0.5-7.0 keV) energy band.
H_Major_Axis_Lo
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent (68% lower confidence limit); ACIS hard
(2.0-7.0 keV) energy band.
M_Major_Axis_Lo
The 1-sigma radius along the major axis of the ellipse defining the
deconvolved source extent (68% lower confidence limit); ACIS medium (1.2-2.0
keV) energy band.
S_Major_Axis_Lo
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent (68% lower confidence limit); ACIS soft
(0.5-1.2 keV) energy band.
U_Major_Axis_Lo
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent (68% lower confidence limit); ACIS ultrasoft
(0.2-0.5 keV) energy band.
W_Major_Axis_Lo
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent (68% lower confidence limit); HRC wide
(~0.1-10.0 keV) energy band.
B_Major_Axis_Hi
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); ACIS broad
(0.5-7.0 keV) energy band.
H_Major_Axis_Hi
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); ACIS hard
(2.0-7.0 keV) energy band.
M_Major_Axis_Hi
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); ACIS medium
(1.2-2.0 keV) energy band.
S_Major_Axis_Hi
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); ACIS soft
(0.5-1.2 keV) energy band.
U_Major_Axis_Hi
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); ACIS ultrasoft
(0.2-0.5 keV) energy band.
W_Major_Axis_Hi
The 1-sigma radius (in arcsec) along the major axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); HRC wide
(~0.1-10.0 keV) energy band.
B_Minor_Axis
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent; ACIS broad (0.5-7.0 keV) energy band.
H_Minor_Axis
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent; ACIS hard (2.0-7.0 keV) energy band.
M_Minor_Axis
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent; ACIS medium (1.2-2.0 keV) energy band.
S_Minor_Axis
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent; ACIS soft (0.5-1.2 keV) energy band.
U_Minor_Axis
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent; ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Minor_Axis
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent; HRC wide (~0.1-10.0 keV) energy band.
B_Minor_Axis_Lo
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% lower confidence limit); ACIS broad
(0.5-7.0 keV) energy band.
H_Minor_Axis_Lo
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% lower confidence limit); ACIS hard
(2.0-7.0 keV) energy band.
M_Minor_Axis_Lo
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% lower confidence limit); ACIS medium
(1.2-2.0 keV) energy band.
S_Minor_Axis_Lo
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% lower confidence limit); ACIS soft
(0.5-1.2 keV) energy band.
U_Minor_Axis_Lo
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% lower confidence limit); ACIS ultrasoft
(0.2-0.5 keV) energy band.
W_Minor_Axis_Lo
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% lower confidence limit); HRC wide
(~0.1-10.0 keV) energy band.
B_Minor_Axis_Hi
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); ACIS broad
(0.5-7.0 keV) energy band.
H_Minor_Axis_Hi
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); ACIS hard
(2.0-7.0 keV) energy band.
M_Minor_Axis_Hi
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); ACIS medium
(1.2-2.0 keV) energy band.
S_Minor_Axis_Hi
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); ACIS soft
(0.5-1.2 keV) energy band.
U_Minor_Axis_Hi
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); ACIS ultrasoft
(0.2-0.5 keV) energy band.
W_Minor_Axis_Hi
The 1-sigma radius (in arcsec) along the minor axis of the ellipse defining
the deconvolved source extent (68% upper confidence limit); HRC wide
(~0.1-10.0 keV) energy band.
B_Position_Angle
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent based on the ACIS broad (0.5-7.0 keV)
energy band, in degrees.
H_Position_Angle
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent based on the ACIS hard (2.0-7.0 keV)
energy band, in degrees.
M_Position_Angle
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent based on the ACIS medium (1.2-2.0 keV)
energy band, in degrees.
S_Position_Angle
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent based on the ACIS soft (0.5-1.2 keV)
energy band, in degrees.
U_Position_Angle
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent based on the ACIS ultrasoft (0.2-0.5
keV) energy band, in degrees.
W_Position_Angle
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent based on the HRC wide (~0.1-10.0 keV)
energy band, in degrees.
B_Position_Angle_Lo
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% lower confidence limit) based on
the ACIS broad (0.5-7.0 keV) energy band, in degrees.
H_Position_Angle_Lo
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% lower confidence limit) based on
the ACIS hard (2.0-7.0 keV) energy band, in degrees.
M_Position_Angle_Lo
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% lower confidence limit) based on
the ACIS medium (1.2-2.0 keV) energy band, in degrees.
S_Position_Angle_Lo
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% lower confidence limit) based on
the ACIS soft (0.5-1.2 keV) energy band, in degrees.
U_Position_Angle_Lo
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% lower confidence limit) based on
the ACIS ultrasoft (0.2-0.5 keV) energy band, in degrees.
W_Position_Angle_Lo
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% lower confidence limit) based on
the HRC wide (~0.1-10.0 keV) energy band, in degrees.
B_Position_Angle_Hi
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% upper confidence limit) based on
the ACIS broad (0.5-7.0 keV) energy band, in degrees.
H_Position_Angle_Hi
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% upper confidence limit) based on
the ACIS hard (2.0-7.0 keV) energy band, in degrees.
M_Position_Angle_Hi
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% upper confidence limit) based on
the ACIS medium (1.2-2.0 keV) energy band, in degrees.
S_Position_Angle_Hi
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% upper confidence limit) based on
the ACIS soft (0.5-1.2 keV) energy band, in degrees.
U_Position_Angle_Hi
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% upper confidence limit) based on
the ACIS ultrasoft (0.2-0.5 keV) energy band, in degrees.
W_Position_Angle_Hi
Position angle (ref. local true north) of the major axis of the ellipse
defining the deconvolved source extent (68% upper confidence limit) based on
the HRC wide (~0.1-10.0 keV) energy band, in degrees.
B_Src_Area
Area (in arcsec2) of the deconvolved source extent ellipse, or area of the
source polygon for extended sources; ACIS broad (0.5-7.0 keV) energy band.
H_Src_Area
Area (in arcsec2) of the deconvolved source extent ellipse, or area of the
source polygon for extended sources; ACIS hard (2.0-7.0 keV) energy band.
M_Src_Area
Area (in arcsec2) of the deconvolved source extent ellipse, or area of the
source polygon for extended sources; ACIS medium (1.2-2.0 keV) energy band.
S_Src_Area
Area (in arcsec2) of the deconvolved source extent ellipse, or area of the
source polygon for extended sources; ACIS soft (0.5-1.2 keV) energy band.
U_Src_Area
Area (in arcsec2) of the deconvolved source extent ellipse, or area of the
source polygon for extended sources; ACIS ultrasoft (0.2-0.5 keV) energy
band.
W_Src_Area
Area (in arcsec2) of the deconvolved source extent ellipse, or area of the
source polygon for extended sources; HRC wide (~0.1-10.0 keV) energy band.
Phot_Nsrcs
Number of sources fit simultaneously to compute aperture photometry
quantities.
B_Photflux_Ap
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0
keV) energy band.
H_Photflux_Ap
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0
keV) energy band.
M_Photflux_Ap
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0
keV) energy band.
S_Photflux_Ap
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2
keV) energy band.
U_Photflux_Ap
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; ACIS ultrasoft
(0.2-0.5 keV) energy band.
W_Photflux_Ap
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0
keV) energy band.
B_Photflux_Ap_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); ACIS broad (0.5-7.0 keV) energy band.
H_Photflux_Ap_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); ACIS hard (2.0-7.0 keV) energy band.
M_Photflux_Ap_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); ACIS medium (1.2-2.0 keV) energy band.
S_Photflux_Ap_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); ACIS soft (0.5-1.2 keV) energy band.
U_Photflux_Ap_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Photflux_Ap_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); HRC wide (~0.1-10.0 keV) energy band.
B_Photflux_Ap_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); ACIS broad (0.5-7.0 keV) energy band.
H_Photflux_Ap_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); ACIS hard (2.0-7.0 keV) energy band.
M_Photflux_Ap_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); ACIS medium (1.2-2.0 keV) energy band.
S_Photflux_Ap_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); ACIS soft (0.5-1.2 keV) energy band.
U_Photflux_Ap_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Photflux_Ap_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); HRC wide (~0.1-10.0 keV) energy band.
B_Photflux_Ap90
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; ACIS broad (0.5-7.0 keV) energy band.
H_Photflux_Ap90
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; ACIS hard (2.0-7.0 keV) energy band.
M_Photflux_Ap90
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; ACIS medium (1.2-2.0 keV) energy band.
S_Photflux_Ap90
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; ACIS soft (0.5-1.2 keV) energy band.
U_Photflux_Ap90
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Photflux_Ap90
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; HRC wide (~0.1-10.0 keV) energy band.
B_Photflux_Ap90_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV)
energy band.
H_Photflux_Ap90_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV)
energy band.
M_Photflux_Ap90_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV)
energy band.
S_Photflux_Ap90_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV)
energy band.
U_Photflux_Ap90_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5
keV) energy band.
W_Photflux_Ap90_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV)
energy band.
B_Photflux_Ap90_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV)
energy band.
H_Photflux_Ap90_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV)
energy band.
M_Photflux_Ap90_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV)
energy band.
S_Photflux_Ap90_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV)
energy band.
U_Photflux_Ap90_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5
keV) energy band.
W_Photflux_Ap90_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
best estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV)
energy band.
B_Flux_Ap
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0
keV) energy band.
H_Flux_Ap
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0
keV) energy band.
M_Flux_Ap
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0
keV) energy band.
S_Flux_Ap
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2
keV) energy band.
U_Flux_Ap
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; ACIS ultrasoft
(0.2-0.5 keV) energy band.
W_Flux_Ap
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events; HRC wide (~0.1-10.0
keV) energy band.
B_Flux_Ap_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Ap_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Ap_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Ap_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Ap_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_Ap_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% lower confidence
limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Ap_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Ap_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Ap_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Ap_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Ap_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_Ap_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, best estimate derived from the longest block of a
multi-band, flux-ordered Bayesian Block analysis of the contributing
observations, and calculated by counting X-ray events (68% upper confidence
limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Ap90
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Ap90
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Ap90
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Ap90
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Ap90
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_Ap90
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events; HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Ap90_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV)
energy band.
H_Flux_Ap90_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV)
energy band.
M_Flux_Ap90_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV)
energy band.
S_Flux_Ap90_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV)
energy band.
U_Flux_Ap90_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5
keV) energy band.
W_Flux_Ap90_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% lower confidence limit); HRC wide (~0.1-10.0 keV)
energy band.
B_Flux_Ap90_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV)
energy band.
H_Flux_Ap90_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV)
energy band.
M_Flux_Ap90_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV)
energy band.
S_Flux_Ap90_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV)
energy band.
U_Flux_Ap90_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5
keV) energy band.
W_Flux_Ap90_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture, best
estimate derived from the longest block of a multi-band, flux-ordered
Bayesian Block analysis of the contributing observations, and calculated by
counting X-ray events (68% upper confidence limit); HRC wide (~0.1-10.0 keV)
energy band.
B_Photflux_Ap_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy band.
H_Photflux_Ap_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy band.
M_Photflux_Ap_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy band.
S_Photflux_Ap_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy band.
U_Photflux_Ap_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy
band.
W_Photflux_Ap_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy band.
B_Photflux_Ap_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% lower confidence limit); ACIS broad
(0.5-7.0 keV) energy band.
H_Photflux_Ap_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% lower confidence limit); ACIS hard
(2.0-7.0 keV) energy band.
M_Photflux_Ap_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% lower confidence limit); ACIS medium
(1.2-2.0 keV) energy band.
S_Photflux_Ap_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% lower confidence limit); ACIS soft
(0.5-1.2 keV) energy band.
U_Photflux_Ap_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% lower confidence limit); ACIS
ultrasoft (0.2-0.5 keV) energy band.
W_Photflux_Ap_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% lower confidence limit); HRC wide
(~0.1-10.0 keV) energy band.
B_Photflux_Ap_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); ACIS broad
(0.5-7.0 keV) energy band.
H_Photflux_Ap_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); ACIS hard
(2.0-7.0 keV) energy band.
M_Photflux_Ap_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); ACIS medium
(1.2-2.0 keV) energy band.
S_Photflux_Ap_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); ACIS soft
(0.5-1.2 keV) energy band.
U_Photflux_Ap_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); ACIS
ultrasoft (0.2-0.5 keV) energy band.
W_Photflux_Ap_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); HRC wide
(~0.1-10.0 keV) energy band.
B_Photflux_Ap90_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; ACIS broad (0.5-7.0 keV) energy band.
H_Photflux_Ap90_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; ACIS hard (2.0-7.0 keV) energy band.
M_Photflux_Ap90_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; ACIS medium (1.2-2.0 keV) energy band.
S_Photflux_Ap90_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; ACIS soft (0.5-1.2 keV) energy band.
U_Photflux_Ap90_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Photflux_Ap90_Avg
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; HRC wide (~0.1-10.0 keV) energy band.
B_Photflux_Ap90_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Photflux_Ap90_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Photflux_Ap90_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Photflux_Ap90_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Photflux_Ap90_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy
band.
W_Photflux_Ap90_Avg_Lo
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Photflux_Ap90_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Photflux_Ap90_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Photflux_Ap90_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Photflux_Ap90_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Photflux_Ap90_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy
band.
W_Photflux_Ap90_Avg_Hi
Aperture-corrected net photon flux, in photons s-1 cm-2, inferred from
the Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Ap_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Ap_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Ap_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Ap_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Ap_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy
band.
W_Flux_Ap_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events; HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Ap_Avg_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% lower confidence limit); ACIS broad
(0.5-7.0 keV) energy band.
H_Flux_Ap_Avg_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% lower confidence limit); ACIS hard
(2.0-7.0 keV) energy band.
M_Flux_Ap_Avg_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% lower confidence limit); ACIS medium
(1.2-2.0 keV) energy band.
S_Flux_Ap_Avg_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% lower confidence limit); ACIS soft
(0.5-1.2 keV) energy band.
U_Flux_Ap_Avg_Lo
Aperture-corrected net energy flux inferred from the source region aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy
band.
W_Flux_Ap_Avg_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% lower confidence limit); HRC wide
(~0.1-10.0 keV) energy band.
B_Flux_Ap_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); ACIS broad
(0.5-7.0 keV) energy band.
H_Flux_Ap_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); ACIS hard
(2.0-7.0 keV) energy band.
M_Flux_Ap_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); ACIS medium
(1.2-2.0 keV) energy band.
S_Flux_Ap_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); ACIS soft
(0.5-1.2 keV) energy band.
U_Flux_Ap_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); ACIS
ultrasoft (0.2-0.5 keV) energy band.
W_Flux_Ap_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
source region aperture, averaged over all contributing observations, and
calculated by counting X-ray events (68% upper confidence limit); HRC wide
(~0.1-10.0 keV) energy band.
B_Flux_Ap90_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Ap90_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Ap90_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Ap90_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Ap90_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_Ap90_Avg
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events; HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Ap90_Avg_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Ap90_Avg_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Ap90_Avg_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Ap90_Avg_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Ap90_Avg_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy
band.
W_Flux_Ap90_Avg_Lo
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Ap90_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Ap90_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Ap90_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Ap90_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Ap90_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy
band.
W_Flux_Ap90_Avg_Hi
Aperture-corrected net energy flux, in erg s-1 cm-2, inferred from the
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture,
averaged over all contributing observations, and calculated by counting X-ray
events (68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_PLaw_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0]; ACIS
broad (0.5-7.0 keV) energy band.
H_Flux_PLaw_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0]; ACIS
hard (2.0-7.0 keV) energy band.
M_Flux_PLaw_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0]; ACIS
medium (1.2-2.0 keV) energy band.
S_Flux_PLaw_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0]; ACIS
soft (0.5-1.2 keV) energy band.
U_Flux_PLaw_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0]; ACIS
ultrasoft (0.2-0.5 keV) energy band.
W_Flux_PLaw_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0]; HRC
wide (~0.1-10.0 keV) energy band.
B_Flux_PLaw_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
lower confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_PLaw_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
lower confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_PLaw_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
lower confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_PLaw_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
lower confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_PLaw_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_PLaw_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
lower confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_PLaw_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
upper confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_PLaw_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
upper confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_PLaw_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
upper confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_PLaw_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
upper confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_PLaw_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_PLaw_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed power law model [NH = NH(Gal); Gamma = 2.0] (68%
upper confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_PLaw_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0]; ACIS broad (0.5-7.0 keV) energy
band.
H_Flux_PLaw_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0]; ACIS hard (2.0-7.0 keV) energy
band.
M_Flux_PLaw_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0]; ACIS medium (1.2-2.0 keV) energy
band.
S_Flux_PLaw_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0]; ACIS soft (0.5-1.2 keV) energy
band.
U_Flux_PLaw_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0]; ACIS ultrasoft (0.2-0.5 keV)
energy band.
W_Flux_PLaw_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0]; HRC wide (~0.1-10.0 keV) energy
band.
B_Flux_PLaw_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS
broad (0.5-7.0 keV) energy band.
H_Flux_PLaw_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS
hard (2.0-7.0 keV) energy band.
M_Flux_PLaw_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS
medium (1.2-2.0 keV) energy band.
S_Flux_PLaw_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS
soft (0.5-1.2 keV) energy band.
U_Flux_PLaw_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% lower confidence limit); ACIS
ultrasoft (0.2-0.5 keV) energy band.
W_Flux_PLaw_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% lower confidence limit); HRC
wide (~0.1-10.0 keV) energy band.
B_Flux_PLaw_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS
broad (0.5-7.0 keV) energy band.
H_Flux_PLaw_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS
hard (2.0-7.0 keV) energy band.
M_Flux_PLaw_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS
medium (1.2-2.0 keV) energy band.
S_Flux_PLaw_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS
soft (0.5-1.2 keV) energy band.
U_Flux_PLaw_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% upper confidence limit); ACIS
ultrasoft (0.2-0.5 keV) energy band.
W_Flux_PLaw_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed power
law model [NH = NH(Gal); Gamma = 2.0] (68% upper confidence limit); HRC
wide (~0.1-10.0 keV) energy band.
B_Flux_BB_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV];
ACIS broad (0.5-7.0 keV) energy band.
H_Flux_BB_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV];
ACIS hard (2.0-7.0 keV) energy band.
M_Flux_BB_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV];
ACIS medium (1.2-2.0 keV) energy band.
S_Flux_BB_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV];
ACIS soft (0.5-1.2 keV) energy band.
U_Flux_BB_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV];
ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_BB_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV];
HRC wide (~0.1-10.0 keV) energy band.
B_Flux_BB_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_BB_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_BB_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_BB_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_BB_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_BB_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_BB_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_BB_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_BB_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_BB_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_BB_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_BB_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed black body model [NH = NH(Gal); kT = 0.75 keV]
(68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_BB_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV]; ACIS broad (0.5-7.0 keV) energy
band.
H_Flux_BB_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV]; ACIS hard (2.0-7.0 keV) energy
band.
M_Flux_BB_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV]; ACIS medium (1.2-2.0 keV)
energy band.
S_Flux_BB_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV]; ACIS soft (0.5-1.2 keV) energy
band.
U_Flux_BB_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV]; ACIS ultrasoft (0.2-0.5 keV)
energy band.
W_Flux_BB_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV]; HRC wide (~0.1-10.0 keV) energy
band.
B_Flux_BB_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% lower confidence limit);
ACIS broad (0.5-7.0 keV) energy band.
H_Flux_BB_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% lower confidence limit);
ACIS hard (2.0-7.0 keV) energy band.
M_Flux_BB_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% lower confidence limit);
ACIS medium (1.2-2.0 keV) energy band.
S_Flux_BB_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% lower confidence limit);
ACIS soft (0.5-1.2 keV) energy band.
U_Flux_BB_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% lower confidence limit);
ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_BB_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% lower confidence limit);
HRC wide (~0.1-10.0 keV) energy band.
B_Flux_BB_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% upper confidence limit);
ACIS broad (0.5-7.0 keV) energy band.
H_Flux_BB_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% upper confidence limit);
ACIS hard (2.0-7.0 keV) energy band.
M_Flux_BB_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% upper confidence limit);
ACIS medium (1.2-2.0 keV) energy band.
S_Flux_BB_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% upper confidence limit);
ACIS soft (0.5-1.2 keV) energy band.
U_Flux_BB_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% upper confidence limit);
ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_BB_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed black
body model [NH = NH(Gal); kT = 0.75 keV] (68% upper confidence limit);
HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Brems_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV];
ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Brems_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV];
ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Brems_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV];
ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Brems_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV];
ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Brems_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV];
ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_Brems_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV];
HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Brems_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Brems_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Brems_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Brems_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Brems_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_Brems_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% lower confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Brems_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Brems_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Brems_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Brems_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Brems_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_Brems_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]
(68% upper confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Brems_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]; ACIS broad (0.5-7.0
keV) energy band.
H_Flux_Brems_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]; ACIS hard (2.0-7.0
keV) energy band.
M_Flux_Brems_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]; ACIS medium (1.2-2.0
keV) energy band.
S_Flux_Brems_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]; ACIS soft (0.5-1.2
keV) energy band.
U_Flux_Brems_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]; ACIS ultrasoft
(0.2-0.5 keV) energy band.
W_Flux_Brems_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV]; HRC wide (~0.1-10.0
keV) energy band.
B_Flux_Brems_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% lower confidence
limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Brems_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% lower confidence
limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Brems_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% lower confidence
limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Brems_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% lower confidence
limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Brems_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% lower confidence
limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_Brems_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% lower confidence
limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_Brems_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% upper confidence
limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_Brems_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% upper confidence
limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_Brems_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% upper confidence
limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_Brems_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% upper confidence
limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_Brems_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% upper confidence
limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_Brems_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed
bremsstrahlung model [NH = NH(Gal); kT = 3.5 keV] (68% upper confidence
limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_APEC_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV]; ACIS
broad (0.5-7.0 keV) energy band.
H_Flux_APEC_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV]; ACIS hard
(2.0-7.0 keV) energy band.
M_Flux_APEC_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV]; ACIS
medium (1.2-2.0 keV) energy band.
S_Flux_APEC_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV]; ACIS soft
(0.5-1.2 keV) energy band.
U_Flux_APEC_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV]; ACIS
ultrasoft (0.2-0.5 keV) energy band.
W_Flux_APEC_Ap
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV]; HRC wide
(~0.1-10.0 keV) energy band.
B_Flux_APEC_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% lower
confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_APEC_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% lower
confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_APEC_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% lower
confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_APEC_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% lower
confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_APEC_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% lower
confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_APEC_Ap_Lo
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% lower
confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_APEC_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% upper
confidence limit); ACIS broad (0.5-7.0 keV) energy band.
H_Flux_APEC_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% upper
confidence limit); ACIS hard (2.0-7.0 keV) energy band.
M_Flux_APEC_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% upper
confidence limit); ACIS medium (1.2-2.0 keV) energy band.
S_Flux_APEC_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% upper
confidence limit); ACIS soft (0.5-1.2 keV) energy band.
U_Flux_APEC_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% upper
confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Flux_APEC_Ap_Hi
Source region aperture model energy flux, in erg s-1 cm-2, inferred from
the canonical absorbed APEC model [NH = NH(Gal); kT = 6.5 keV] (68% upper
confidence limit); HRC wide (~0.1-10.0 keV) energy band.
B_Flux_APEC_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV]; ACIS broad (0.5-7.0 keV) energy band.
H_Flux_APEC_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV]; ACIS hard (2.0-7.0 keV) energy band.
M_Flux_APEC_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV]; ACIS medium (1.2-2.0 keV) energy
band.
S_Flux_APEC_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV]; ACIS soft (0.5-1.2 keV) energy band.
U_Flux_APEC_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV]; ACIS ultrasoft (0.2-0.5 keV) energy
band.
W_Flux_APEC_Ap90
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV]; HRC wide (~0.1-10.0 keV) energy band.
B_Flux_APEC_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS
broad (0.5-7.0 keV) energy band.
H_Flux_APEC_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS
hard (2.0-7.0 keV) energy band.
M_Flux_APEC_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS
medium (1.2-2.0 keV) energy band.
S_Flux_APEC_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS
soft (0.5-1.2 keV) energy band.
U_Flux_APEC_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% lower confidence limit); ACIS
ultrasoft (0.2-0.5 keV) energy band.
W_Flux_APEC_Ap90_Lo
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% lower confidence limit); HRC wide
(~0.1-10.0 keV) energy band.
B_Flux_APEC_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS
broad (0.5-7.0 keV) energy band.
H_Flux_APEC_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS
hard (2.0-7.0 keV) energy band.
M_Flux_APEC_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS
medium (1.2-2.0 keV) energy band.
S_Flux_APEC_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS
soft (0.5-1.2 keV) energy band.
U_Flux_APEC_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% upper confidence limit); ACIS
ultrasoft (0.2-0.5 keV) energy band.
W_Flux_APEC_Ap90_Hi
Point Spread Function (PSF) 90% Enclosed Counts Fraction (ECF) aperture model
energy flux, in erg s-1 cm-2, inferred from the canonical absorbed APEC
model [NH = NH(Gal); kT = 6.5 keV] (68% upper confidence limit); HRC wide
(~0.1-10.0 keV) energy band.
Likelihood
Highest detection log likelihood across all stacked observations and energy
bands.
Likelihood_Class
Highest detection likelihood classification across all stacked observations
and energy bands.
Significance
Highest flux significance (S/N) across all stacked observations and energy
bands.
Flux_Plaw
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed power-law model spectrum to the source region aperture PI
spectrum.
Flux_PLaw_Lo
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed power-law model spectrum to the source region aperture PI
spectrum (68% lower confidence limit).
Flux_PLaw_Hi
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed power-law model spectrum to the source region aperture PI
spectrum (68% upper confidence limit).
PowLaw_Gamma
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_Lo
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).
PowLaw_Gamma_Hi
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).
PowLaw_Gamma_Rhat
Photon index convergence criterion of the best fitting absorbed power-law
model spectrum to the source region aperture PI spectrum.
PowLaw_NH
NH column density, in units of 1020 cm-2, of the best fitting absorbed
power-law model spectrum to the source region aperture PI spectrum.
PowLaw_NH_Lo
NH column density, in units of 1020 cm-2, of the best fitting absorbed
power-law model spectrum to the source region aperture PI spectrum (68% lower
confidence limit).
PowLaw_NH_Hi
NH column density, in units of 1020 cm-2, of the best fitting absorbed
power-law model spectrum to the source region aperture PI spectrum (68% upper
confidence limit).
PowLaw_NH_Rhat
NH column density convergence criterion of the best fitting absorbed
power-law model spectrum to the source region aperture PI spectrum.
PowLaw_Ampl
Amplitude of the best fitting absorbed power-law model spectrum to the source
region aperture PI spectrum.
PowLaw_Ampl_Lo
Amplitude of the best fitting absorbed power-law model spectrum to the source
region aperture PI spectrum (68% lower confidence limit).
PowLaw_Ampl_Hi
Amplitude of the best fitting absorbed power-law model spectrum to the source
region aperture PI spectrum (68% upper confidence limit).
PowLaw_Ampl_Rhat
Amplitude convergence criterion of the best fitting absorbed power-law model
spectrum to the source region aperture PI spectrum.
PowLaw_Stat
chi-square statistic per degree of freedom of the best fitting absorbed
power-law model spectrum to the source region aperture PI spectrum.
Flux_BB
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed black body model spectrum to the source region aperture PI
spectrum.
Flux_BB_Lo
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed black body model spectrum to the source region aperture PI
spectrum (68% lower confidence limit).
Flux_BB_Hi
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed black body model spectrum to the source region aperture PI
spectrum (68% upper confidence limit).
BB_kT
Temperature (kT) of the best fitting absorbed black body model spectrum to
the source region aperture PI spectrum.
BB_kT_Lo
Temperature (kT) of the best fitting absorbed black body model spectrum to
the source region aperture PI spectrum (68% lower confidence limit).
BB_kT_Hi
Temperature (kT) of the best fitting absorbed black body model spectrum to
the source region aperture PI spectrum (68% upper confidence limit).
BB_kT_Rhat
Temperature (kT) convergence criterion of the best fitting absorbed black
body model spectrum to the source region aperture PI spectrum.
BB_NH
NH column density, in units of 1020 cm-2, of the best fitting absorbed
black body model spectrum to the source region aperture PI spectrum.
BB_NH_Lo
NH column density, in units of 1020 cm-2, of the best fitting absorbed
black body model spectrum to the source region aperture PI spectrum (68%
lower confidence limit).
BB_NH_Hi
NH column density, in units of 1020 cm-2, of the best fitting absorbed
black body model spectrum to the source region aperture PI spectrum (68%
upper confidence limit).
BB_NH_Rhat
NH column density convergence criterion of the best fitting absorbed black
body model spectrum to the source region aperture PI spectrum.
BB_Ampl
Amplitude of the best fitting absorbed black body model spectrum to the
source region aperture PI spectrum.
BB_Ampl_Lo
Amplitude of the best fitting absorbed black body model spectrum to the
source region aperture PI spectrum (68% lower confidence limit).
BB_Ampl_Hi
Amplitude of the best fitting absorbed black body model spectrum to the
source region aperture PI spectrum (68% upper confidence limit).
BB_Ampl_Rhat
Amplitude convergence criterion of the best fitting absorbed black body model
spectrum to the source region aperture PI spectrum.
BB_Stat
chi-square statistic per degree of freedom of the best fitting absorbed black
body model spectrum to the source region aperture PI spectrum.
Flux_Brems
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed bremsstrahlung model spectrum to the source region aperture
PI spectrum.
Flux_Brems_Lo
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed bremsstrahlung model spectrum to the source region aperture
PI spectrum (68% lower confidence limit).
Flux_Brems_Hi
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed bremsstrahlung model spectrum to the source region aperture
PI spectrum (68% upper confidence limit).
Brems_kT
Temperature (kT) of the best fitting absorbed bremsstrahlung model spectrum
to the source region aperture PI spectrum.
Brems_kT_Lo
Temperature (kT) of the best fitting absorbed bremsstrahlung model spectrum
to the source region aperture PI spectrum (68% lower confidence limit).
Brems_kT_Hi
Temperature (kT) of the best fitting absorbed bremsstrahlung model spectrum
to the source region aperture PI spectrum (68% upper confidence limit).
Brems_kT_Rhat
Temperature (kT) convergence criterion of the best fitting absorbed
bremsstrahlung model spectrum to the source region aperture PI spectrum.
Brems_NH
NH column density, in units of 1020 cm-2, of the best fitting absorbed
bremsstrahlung model spectrum to the source region aperture PI spectrum.
Brems_NH_Lo
NH column density, in units of 1020 cm-2, of the best fitting absorbed
bremsstrahlung model spectrum to the source region aperture PI spectrum (68%
lower confidence limit).
Brems_NH_Hi
NH column density, in units of 1020 cm-2, of the best fitting absorbed
bremsstrahlung model spectrum to the source region aperture PI spectrum (68%
upper confidence limit).
Brems_NH_Rhat
NH column density convergence criterion of the best fitting absorbed
bremsstrahlung model spectrum to the source region aperture PI spectrum.
Brems_Norm
Amplitude of the best fitting absorbed bremsstrahlung model spectrum to the
source region aperture PI spectrum.
Brems_Norm_Lo
Amplitude of the best fitting absorbed bremsstrahlung model spectrum to the
source region aperture PI spectrum (68% lower confidence limit).
Brems_Norm_Hi
Amplitude of the best fitting absorbed bremsstrahlung model spectrum to the
source region aperture PI spectrum (68% upper confidence limit).
Brems_Norm_Rhat
Amplitude convergence criterion of the best fitting absorbed bremsstrahlung
model spectrum to the source region aperture PI spectrum.
Brems_Stat
chi-square statistic per degree of freedom of the best fitting absorbed
bremsstrahlung model spectrum to the source region aperture PI spectrum.
Flux_APEC
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed APEC model spectrum to the source region aperture PI
spectrum.
Flux_APEC_Lo
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed APEC model spectrum to the source region aperture PI
spectrum (68% lower confidence limit).
Flux_APEC_Hi
Net integrated 0.5-7.0 keV energy flux, in erg s-1 cm-2, of the best
fitting absorbed APEC model spectrum to the source region aperture PI
spectrum (68% upper confidence limit).
APEC_kT
Temperature (kT) of the best fitting absorbed APEC model spectrum to the
source region aperture PI spectrum.
APEC_kT_Lo
Temperature (kT) of the best fitting absorbed APEC model spectrum to the
source region aperture PI spectrum (68% lower confidence limit).
APEC_kT_Hi
Temperature (kT) of the best fitting absorbed APEC model spectrum to the
source region aperture PI spectrum (68% upper confidence limit).
APEC_kT_Rhat
Temperature (kT) convergence criterion of the best fitting absorbed APEC
model spectrum to the source region aperture PI spectrum.
APEC_Abund
Abundance of the best fitting absorbed APEC model spectrum to the source
region aperture PI spectrum.
APEC_Abund_Lo
Abundance of the best fitting absorbed APEC model spectrum to the source
region aperture PI spectrum (68% lower confidence limit).
APEC_Abund_Hi
Abundance of the best fitting absorbed APEC model spectrum to the source
region aperture PI spectrum (68% upper confidence limit).
APEC_Abund_Rhat
Abundance convergence criterion of the best fitting absorbed APEC model
spectrum to the source region aperture PI spectrum.
APEC_Z
Redshift of the best fitting absorbed APEC model spectrum to the source
region aperture PI spectrum.
APEC_Z_Lo
Redshift of the best fitting absorbed APEC model spectrum to the source
region aperture PI spectrum (68% lower confidence limit).
APEC_Z_Hi
Redshift of the best fitting absorbed APEC model spectrum to the source
region aperture PI spectrum (68% upper confidence limit).
APEC_Z_Rhat
Redshift convergence criterion Redshift of the best fitting absorbed APEC
model spectrum to the source region aperture PI spectrum.
APEC_NH
NH column density, in units of 1020 cm-2, of the best fitting absorbed
APEC model spectrum to the source region aperture PI spectrum.
APEC_NH_Lo
NH column density, in units of 1020 cm-2, of the best fitting absorbed
APEC model spectrum to the source region aperture PI spectrum (68% lower
confidence limit).
APEC_NH_Hi
NH column density, in units of 1020 cm-2, of the best fitting absorbed
APEC model spectrum to the source region aperture PI spectrum (68% upper
confidence limit).
APEC_NH_Rhat
NH column density convergence criterion of the best fitting absorbed APEC
model spectrum to the source region aperture PI spectrum.
APEC_Norm
Amplitude of the best fitting absorbed APEC model spectrum to the source
region aperture PI spectrum.
APEC_Norm_Lo
Amplitude of the best fitting absorbed APEC model spectrum to the source
region aperture PI spectrum (68% lower confidence limit).
APEC_Norm_Hi
Amplitude of the best fitting absorbed APEC model spectrum to the source
region aperture PI spectrum (68% upper confidence limit).
APEC_Norm_Rhat
Amplitude convergence criterion of the best fitting absorbed APEC model
spectrum to the source region aperture PI spectrum.
APEC_Stat
chi-square statistic per degree of freedom of the best fitting absorbed APEC
model spectrum to the source region aperture PI spectrum.
NH_Gal
Galactic NH column density, in units of 1020 cm-2, in direction of
source.
Hardness_Ratio_HM
ACIS hard (2-7 keV) - medium (1.2-2.0 keV) energy band hardness ratio.
Hardness_Ratio_HM_Lo
ACIS hard (2-7 keV) - medium (1.2-2.0 keV) energy band hardness ratio (68%
lower confidence limit).
Hardness_Ratio_HM_Hi
ACIS hard (2-7 keV) - medium (1.2-2.0 keV) energy band hardness ratio (68%
upper confidence limit).
Var_Inter_Hard_Prob_Hm
Inter-observation ACIS hard (2-7 keV) - medium (1.2-2.0 keV) energy band
hardness ratio variability probability.
Var_Inter_Hard_Sigma_Hm
Inter-observation ACIS hard (2-7 keV) - medium (1.2-2.0 keV) energy band
hardness ratio variability standard deviation.
Hardness_Ratio_HS
ACIS hard (2-7 keV) - soft (0.5-1.2 keV) energy band hardness ratio.
Hardness_Ratio_HS_Lo
ACIS hard (2-7 keV) - soft (0.5-1.2 keV) energy band hardness ratio (68%
lower confidence limit).
Hardness_Ratio_HS_Hi
ACIS hard (2-7 keV) - soft (0.5-1.2 keV) energy band hardness ratio (68%
upper confidence limit).
Var_Inter_Hard_Prob_Hs
Inter-observation ACIS hard (2-7 keV) - soft (0.5-1.2 keV) energy band
hardness ratio variability probability.
Var_Inter_Hard_Sigma_Hs
Inter-observation ACIS hard (2-7 keV) - soft (0.5-1.2 keV) energy band
hardness ratio variability standard deviation.
Hardness_Ratio_MS
ACIS medium (1.2-2.0 keV) - soft (0.5-1.2 keV) energy band hardness ratio.
Hardness_Ratio_MS_Lo
ACIS medium (1.2-2.0 keV) - soft (0.5-1.2 keV) energy band hardness ratio
(68% lower confidence limit).
Hardness_Ratio_MS_Hi
ACIS medium (1.2-2.0 keV) - soft (0.5-1.2 keV) energy band hardness ratio
(68% upper confidence limit).
Var_Inter_Hard_Prob_Ms
Inter-observation ACIS medium (1.2-2.0 keV) - soft (0.5-1.2 keV) energy band
hardness ratio variability probability.
Var_Inter_Hard_Sigma_Ms
Inter-observation ACIS medium (1.2-2.0 keV) - soft (0.5-1.2 keV) energy band
hardness ratio variability standard deviation.
B_Ks_Intra_Prob
Intra-observation Kolmogorov-Smirnov test variability probability (highest
value across all observations); ACIS broad (0.5-7.0 keV) energy band.
H_Ks_Intra_Prob
Intra-observation Kolmogorov-Smirnov test variability probability (highest
value across all observations); ACIS hard (2.0-7.0 keV) energy band.
M_Ks_Intra_Prob
Intra-observation Kolmogorov-Smirnov test variability probability (highest
value across all observations); ACIS medium (1.2-2.0 keV) energy band.
S_Ks_Intra_Prob
Intra-observation Kolmogorov-Smirnov test variability probability (highest
value across all observations); ACIS soft (0.5-1.2 keV) energy band.
U_Ks_Intra_Prob
Intra-observation Kolmogorov-Smirnov test variability probability (highest
value across all observations); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Ks_Intra_Prob
Intra-observation Kolmogorov-Smirnov test variability probability (highest
value across all observations); HRC wide (~0.1-10.0 keV) energy band.
B_Kp_Intra_Prob
Intra-observation Kuiper's test variability probability (highest value across
all observations); ACIS broad (0.5-7.0 keV) energy band.
H_Kp_Intra_Prob
Intra-observation Kuiper's test variability probability (highest value across
all observations); ACIS hard (2.0-7.0 keV) energy band.
M_Kp_Intra_Prob
Intra-observation Kuiper's test variability probability (highest value across
all observations); ACIS medium (1.2-2.0 keV) energy band.
S_Kp_Intra_Prob
Intra-observation Kuiper's test variability probability (highest value across
all observations); ACIS soft (0.5-1.2 keV) energy band.
U_Kp_Intra_Prob
Intra-observation Kuiper's test variability probability (highest value across
all observations); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Kp_Intra_Prob
Intra-observation Kuiper's test variability probability (highest value across
all observations); HRC wide (~0.1-10.0 keV) energy band.
B_Var_Intra_Prob
Intra-observation Gregory-Loredo variability probability (highest value
across all observations); ACIS broad (0.5-7.0 keV) energy band.
H_Var_Intra_Prob
Intra-observation Gregory-Loredo variability probability (highest value
across all observations); ACIS hard (2.0-7.0 keV) energy band.
M_Var_Intra_Prob
Intra-observation Gregory-Loredo variability probability (highest value
across all observations); ACIS medium (1.2-2.0 keV) energy band.
S_Var_Intra_Prob
Intra-observation Gregory-Loredo variability probability (highest value
across all observations); ACIS soft (0.5-1.2 keV) energy band.
U_Var_Intra_Prob
Intra-observation Gregory-Loredo variability probability (highest value
across all observations); ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Var_Intra_Prob
Intra-observation Gregory-Loredo variability probability (highest value
across all observations); HRC wide (~0.1-10.0 keV) energy band.
B_Var_Intra_Index
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 (0.5-7.0 keV)
energy band.
H_Var_Intra_Index
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 (2.0-7.0 keV)
energy band.
M_Var_Intra_Index
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 (1.2-2.0
keV) energy band.
S_Var_Intra_Index
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 (0.5-1.2 keV)
energy band.
U_Var_Intra_Index
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 (0.2-0.5
keV) energy band.
W_Var_Intra_Index
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 (~0.1-10.0 keV)
energy band.
B_Var_Inter_Prob
Inter-observation variability probability, calculated from the chi2
distribution of the photon fluxes of the individual observations; ACIS broad
(0.5-7.0 keV) energy band.
H_Var_Inter_Prob
Inter-observation variability probability, calculated from the chi2
distribution of the photon fluxes of the individual observations; ACIS hard
(2.0-7.0 keV) energy band.
M_Var_Inter_Prob
Inter-observation variability probability, calculated from the chi2
distribution of the photon fluxes of the individual observations; ACIS medium
(1.2-2.0 keV) energy band.
S_Var_Inter_Prob
Inter-observation variability probability, calculated from the chi2
distribution of the photon fluxes of the individual observations; ACIS soft
(0.5-1.2 keV) energy band.
U_Var_Inter_Prob
Inter-observation variability probability, calculated from the chi2
distribution of the photon fluxes of the individual observations; ACIS
ultrasoft (0.2-0.5 keV) energy band.
W_Var_Inter_Prob
Inter-observation variability probability, calculated from the chi2
distribution of the photon fluxes of the individual observations; HRC wide
(~0.1-10.0 keV) energy band.
B_Var_Inter_Index
Inter-observation variability index in the range [0, 10]: indicates whether
the source region photon flux is constant between observations; ACIS broad
(0.5-7.0 keV) energy band.
H_Var_Inter_Index
Inter-observation variability index in the range [0, 10]: indicates whether
the source region photon flux is constant between observations; ACIS hard
(2.0-7.0 keV) energy band.
M_Var_Inter_Index
Inter-observation variability index in the range [0, 10]: indicates whether
the source region photon flux is constant between observations; ACIS medium
(1.2-2.0 keV) energy band.
S_Var_Inter_Index
Inter-observation variability index in the range [0, 10]: indicates whether
the source region photon flux is constant between observations; ACIS soft
(0.5-1.2 keV) energy band.
U_Var_Inter_Index
Inter-observation variability index in the range [0, 10]: indicates whether
the source region photon flux is constant between observations; ACIS
ultrasoft (0.2-0.5 keV) energy band.
W_Var_Inter_Index
Inter-observation variability index in the range [0, 10]: indicates whether
the source region photon flux is constant between observations; HRC wide
(~0.1-10.0 keV) energy band.
B_Var_Inter_Sigma
Inter-observation flux variability standard deviation, in photons s-1
cm-2; the spread of the individual observation photon fluxes about the
error weighted mean; ACIS broad (0.5-7.0 keV) energy band.
H_Var_Inter_Sigma
Inter-observation flux variability standard deviation, in photons s-1
cm-2; the spread of the individual observation photon fluxes about the
error weighted mean; ACIS hard (2.0-7.0 keV) energy band.
M_Var_Inter_Sigma
Inter-observation flux variability standard deviation, in photons s-1
cm-2; the spread of the individual observation photon fluxes about the
error weighted mean; ACIS medium (1.2-2.0 keV) energy band.
S_Var_Inter_Sigma
Inter-observation flux variability standard deviation, in photons s-1
cm-2; the spread of the individual observation photon fluxes about the
error weighted mean; ACIS soft (0.5-1.2 keV) energy band.
U_Var_Inter_Sigma
Inter-observation flux variability standard deviation, in photons s-1
cm-2; the spread of the individual observation photon fluxes about the
error weighted mean; ACIS ultrasoft (0.2-0.5 keV) energy band.
W_Var_Inter_Sigma
Inter-observation flux variability standard deviation, in photons s-1
cm-2; the spread of the individual observation photon fluxes about the
error weighted mean; HRC wide (~0.1-10.0 keV) energy band.
Dither_Warning_Flag
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.
ACIS_Num
Total number of ACIS imaging observations contributing to the Master Sources
Table record of the source.
ACIS_HETG_Num
Total number of ACIS/HETG observations contributing to the Master Sources
Table record of the source.
ACIS_LETG_Num
Total number of ACIS/LETG observations contributing to the Master Sources
Table record of the source.
ACIS_Time
Total livetime (in seconds) for all ACIS imaging observations contributing to
the Master Sources Table record of the source.
ACIS_HETG_Time
Total livetime (in seconds) for all ACIS/HETG observations contributing to
the Master Sources Table record of the source.
ACIS_LETG_Time
Total livetime (in seconds) for all ACIS/LETG observations contributing to
the Master Sources Table record of the source.
HRC_Num
Total number of HRC imaging observations contributing to the Master Sources
Table record of the source.
HRC_HETG_Num
Total number of HRC/HETG observations contributing to the Master Sources
Table record of the source.
HRC_LETG_Num
Total number of HRC/LETG observations contributing to the Master Sources
Table record of the source.
HRC_Time
Total livetime (in seconds) for all HRC imaging observations contributing to
the Master Sources Table record of the source.
HRC_HETG_Time
Total livetime (in seconds) for all HRC/HETG observations contributing to the
Master Sources Table record of the source.
HRC_LETG_Time
Total livetime (in seconds) for all HRC/LETG observations contributing to the
Master Sources Table record of the source.
Contact Person
Questions regarding the CSC database table can be addressed to the HEASARC Help Desk.Page Author: Browse Software Development Team
Last Modified: Monday, 16-Sep-2024 17:26:27 EDT
- HEASARC Director: Dr. Andy Ptak
- NASA Official: Dr. Andy Ptak
- Web Curator: J.D. Myers
- Last Modified: 16-Sep-2024