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 X083631.99-430612.4 chandra ccd3 146.78 638.053 40.1849 6.33916 0.0387771 0.00611707 86.024 1 3.75317 2.31369 146.008 8.42044 F F 1.01e+22 6.79327e-13 1 dsx
Report srcpi bgdpi arf 1 X083611.91-431330.2 chandra ccd2 717.833 807.389 8.89809 3 0.00858632 0.00289489 19.0363 1 0.616816 0.546499 130.269 3.38133 F F 1.01e+22 1.3211e-13 1 dx
Report 3 X083555.48-431108.6 chandra ccd3 958.9 36.2998 4.97284 2.23607 0.00479861 0.00215772 10.6454 1 0.492 0.492 83.7356 0.501534 F F 1.01e+22 0 1 d
Report srcpi bgdpi arf 2 X083628.09-430417.7 chandra ccd3 232.7 870.9 4.03347 2.2361 0.00389215 0.00215775 8.63448 0.999997 2.22722 0.870782 174.622 9.30231 A F 1.01e+22 6.89583e-14 1 dx

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