Source List

Observation details report
Detailed source parameters (including errors) in a comma-separated values file

Click on source number for detailed analysis, including spectral fits if applicable

data idnum idradec telescope instrument x y cnts cntserr rate rateerr SNR poisprob sigmaj sigmin incang offax cnts_soft cnts_hard hr hr_err ext var N_H flux vign flags
Report srcpi bgdpi arf 1 X095406.60-050452.5 chandra ccd0 553.913 973.854 11.7696 3.43069 0.00482681 0.00140695 30.3885 1 2.31639 2.31639 0 7.70764 F F 3.05e+20 6.75734e-14 1 dsx
Report srcpi bgdpi arf 1 X095317.89-050224.2 chandra ccd3 589.5 1223.9 4.82114 2.23607 0.00197716 0.000917018 12.0676 0.999999 1.19875 0.581844 48.7035 6.25368 A F 3.14e+20 2.76751e-14 1 dx
Report 2 X095310.36-050541.5 chandra ccd3 818 822.75 3.95664 2 0.00162263 0.000820204 9.9037 0.999999 0.928683 0.492 111.697 6.55988 A F 3.19e+20 0 1 d
Report srcpi bgdpi arf 2 X095406.90-050818.1 chandra ccd0 544.167 555.5 2.91355 1.73205 0.00119485 0.000710319 7.52263 0.999981 0.781389 0.492 14.6789 7.76859 A F 3.08e+20 1.61836e-14 1 dx
Report 1 X095335.54-051246.3 chandra ccd1 790.5 701.5 0.977022 1 0.000401189 0.000410624 2.30332 0.98563 0.492 0.492 90 6.15823 F F 3.21e+20 0 1 d
Report 1 X095340.18-045702.1 chandra ccd2 676.5 1156.5 0.902874 1 0.00037027 0.000410104 2.2439 0.988226 0.492 0.492 90 9.62679 F F 3.06e+20 0 1 d

counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 7.99 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), T = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters, b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters, i = psf spatial fitting parameters, f = spectral fitting parameters, c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest