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 X205257.57-063944.4 chandra ccd3 279.9 384.4 9.49614 3.16229 0.00574685 0.00191375 30.4299 1 2.8779 0.926389 126.11 9.58586 A F 4.52e+20 7.49813e-14 1 dx
Report srcpi bgdpi arf 2 X205328.88-063820.5 chandra ccd7 651.944 121.944 8.9339 3 0.0054066 0.00181553 19.1845 1 0.590541 0.492 132.08 2.30098 F F 4.44e+20 3.97421e-14 1 dx
Report srcpi bgdpi arf 1 X205358.93-064505.6 chandra ccd5 631.056 1221.5 7.58754 3.00004 0.00459181 0.00181556 13.9503 1 2.48218 2.0322 116.774 10.726 F F 4.35e+20 4.19111e-14 1 dx
Report srcpi bgdpi arf 2 X205346.37-064121.8 chandra ccd6 524.25 665.5 3.91991 2 0.00237224 0.00121036 12.6233 1 0.876141 0.492 116.821 5.88777 A F 4.38e+20 2.62729e-14 1 dx
Report 1 X205333.30-063210.3 chandra ccd7 518.167 874.5 2.96687 1.73205 0.00179548 0.0010482 6.371 0.999922 0.492 0.492 40.2688 4.21208 F F 4.41e+20 0 1 d
Report 1 X205348.38-064110.0 chandra ccd6 463.5 689.5 1.93932 1.41422 0.00117364 0.000855852 6.2452 0.999861 1.04369 0.492 45 6.0099 A F 4.38e+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