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 4 X083551.95-505811.1 chandra ccd3 95.8385 77.1919 422.669 20.8926 0.135955 0.00672028 113.65 1 0.430818 0.377806 42.6246 0.266536 F F 4.69e+21 0 1 ds
Report 1 X083617.45-510005.9 chandra ccd0 588.1 913.1 4.93114 2.23607 0.00158612 0.000719241 13.0062 1 0.619274 0.492 107.496 4.17982 F F 4.74e+21 0 1 d
Report 3 X083534.63-510004.4 chandra ccd1 377.5 875.25 3.96122 2 0.00127414 0.000643309 9.86465 0.999999 0.492 0.492 50.3098 3.47179 F T 4.6e+21 0 1 d
Report 1 X083516.38-510041.9 chandra ccd1 727.5 798.5 3.77021 2.00001 0.0012127 0.000643311 9.38899 0.999975 1.20132 0.492 129.345 6.32505 A F 4.54e+21 0 1 d
Report 2 X083608.26-510050.1 chandra ccd0 764.5 823.5 2.98686 1.73205 0.000960738 0.000557122 7.87806 0.999984 0.492 0.492 90 3.44828 F F 4.71e+21 0 1 d
Report 2 X083529.06-505913.8 chandra ccd1 484.5 978 1.98619 1.41421 0.000638868 0.000454888 4.94624 0.999381 0.492 0.492 26.5651 3.96567 F F 4.59e+21 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