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 rmf 5 X202420.55-572343.5 chandra ccd7 724.105 446.249 463.87 22.1102 0.17905 0.00853435 130.866 1 0.487192 0.416826 125.081 0.578079 F F 5.01e+20 2.82937e-12 1 dsxf
Report srcpi bgdpi arf 1 X202354.87-572134.9 chandra ccd7 1146.33 707.245 12.5779 3.56593 0.00485495 0.00137641 3.54846 0.999401 1.20634 1.20634 0 4.10383 F T 4.97e+20 3.84173e-14 1 dsx
Report srcpi bgdpi arf 1 X202419.21-572722.9 chandra ccd6 367.667 947.667 5.92927 2.44949 0.00218216 0.000901492 14.0757 1 0.526599 0.492 122.612 3.17043 F T 4.97e+20 2.15239e-14 1 dx
Report 2 X202403.46-572804.8 chandra ccd6 625.833 862.5 2.97152 1.73205 0.00109362 0.000637451 7.05418 0.999964 0.529672 0.492 100.278 4.34894 F F 4.92e+20 0 1 d
Report 3 X202404.66-572711.0 chandra ccd6 606.25 971.75 3.97374 2 0.00146247 0.000736065 9.43337 0.999999 0.492 0.492 45 3.48925 F F 4.93e+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