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Last modified: 27 March 2023

URL: https://cxc.cfa.harvard.edu/csc/columns/chs_properties.html

Properties of Convex-Hull Sources in CSC 2.0

Convex-hull sources - representing large, or irregular, X-ray sources that are much larger than the Chandra PSF - are new in release 2.0 of the CSC, and should be considered an alpha release. Only a small-number of the properties calculated for compact sources - given in the master source table - are calculated for convex-hull sources. The Convex-Hull pipeline page outlines the steps taken in calculating the properties and the following table lists these columns:

Master Source properties that are populated for convex-hull sources
Column name Description
name Source name in the format '2CXO Jhhmmss.s{+|-}ddmmss[X]'
ra Source position, ICRS right ascension
dec Source position, ICRS declination
err_ellipse_r0 Major radius of the 95% confidence level position error ellipse
err_ellipse_r1 Minor radius of the 95% confidence level position error ellipse
err_ellipse_ang Position angle (ref. local true north) of the major axis of the 95% confidence level error ellipse
gal_b Source position, Galactic latitude (equinox J2000.0, epoch J2000.0)
gal_l Source position, Galactic longitude (equinox J2000.0, epoch J2000.0)
extent_flag Source is extended, or deconvolved source extent is inconsistent with a point source at the 90% confidence level in one or more observations and energy bands
streak_src_flag Source is located on an ACIS readout streak in all observations; source properties may be affected
man_add_flag Source was manually added in the catalog via human review
man_inc_flag Source was manually included in the catalog via human review (detection was rejected by automated criteria)
man_reg_flag Source region parameters (dimensions, initial guess position input to the Maximum Likelihood Estimator fit) were manually modified via human review
man_match_flag Source detections were manually matched between overlapping stacked observations via human review
man_pos_flag Best fit source position was manually modified via human review
src_area_b Area of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS broad (0.5-7.0 keV) energy band
src_area_h Area of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS hard (2.0-7.0 keV) energy band
src_area_m Area of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS medium (1.2-2.0 keV) energy band
src_area_s Area of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS soft (0.5-1.2 keV) energy band
src_area_u Area of the deconvolved source extent ellipse, or area of the source polygon for extended sources; ACIS ultrasoft (0.2-0.5 keV) energy band
phot_nsrcs Number of sources fit simultaneously to compute aperture photometry quantities
photflux_aper_avg_b Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy band
photflux_aper_avg_h Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy band
photflux_aper_avg_m Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy band
photflux_aper_avg_s Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy band
photflux_aper_avg_u Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy band
photflux_aper_avg_lolim_b Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS broad (0.5-7.0 keV) energy band
photflux_aper_avg_lolim_h Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS hard (2.0-7.0 keV) energy band
photflux_aper_avg_lolim_m Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS medium (1.2-2.0 keV) energy band
photflux_aper_avg_lolim_s Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS soft (0.5-1.2 keV) energy band
photflux_aper_avg_lolim_u Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% lower confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
photflux_aper_avg_hilim_b Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
photflux_aper_avg_hilim_h Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
photflux_aper_avg_hilim_m Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
photflux_aper_avg_hilim_s Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
photflux_aper_avg_hilim_u Aperture-corrected net photon flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy band
flux_aper_avg_b Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS broad (0.5-7.0 keV) energy band
flux_aper_avg_h Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS hard (2.0-7.0 keV) energy band
flux_aper_avg_m Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS medium (1.2-2.0 keV) energy band
flux_aper_avg_s Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS soft (0.5-1.2 keV) energy band
flux_aper_avg_u Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events; ACIS ultrasoft (0.2-0.5 keV) energy band
flux_aper_avg_lolim_b 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 broad (0.5-7.0 keV) energy band
flux_aper_avg_lolim_h 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 hard (2.0-7.0 keV) energy band
flux_aper_avg_lolim_m 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 medium (1.2-2.0 keV) energy band
flux_aper_avg_lolim_s 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 soft (0.5-1.2 keV) energy band
flux_aper_avg_lolim_u 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
flux_aper_avg_hilim_b Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS broad (0.5-7.0 keV) energy band
flux_aper_avg_hilim_h Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS hard (2.0-7.0 keV) energy band
flux_aper_avg_hilim_m Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS medium (1.2-2.0 keV) energy band
flux_aper_avg_hilim_s Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS soft (0.5-1.2 keV) energy band
flux_aper_avg_hilim_u Aperture-corrected net energy flux inferred from the source region aperture, averaged over all contributing observations, and calculated by counting X-ray events (68% upper confidence limit); ACIS ultrasoft (0.2-0.5 keV) energy 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
nh_gal Galactic N_H column density in direction of source
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 for all ACIS imaging 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