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 4 X202749.86-550736.5 chandra ccd7 180.913 644.104 21.6263 4.66433 0.0106998 0.00230773 40.0734 1 0.795108 0.248758 318.697 3.31814 A F 4.09e+20 8.74803e-14 1 dsx
Report srcpi bgdpi arf 3 X202716.55-550904.5 chandra ccd7 760.833 464.722 8.928 3 0.00441714 0.00148426 16.5435 1 0.548471 0.492 31.5171 4.72514 F F 4.14e+20 3.84433e-14 1 dx
Report srcpi bgdpi arf 1 X202742.28-550150.5 chandra ccd6 1074.25 564 7.96252 2.82843 0.00393963 0.00139943 22.3449 1 0.514845 0.492 175.787 3.45334 F F 4.04e+20 4.28911e-14 1 dx
Report srcpi bgdpi arf 1 X202724.92-550522.4 chandra ccd7 615.25 916.25 3.94941 2 0.00195398 0.000989504 7.31824 0.999986 0.492 0.492 163.997 1.404 F F 4.09e+20 1.46591e-14 1 dx
Report 2 X202718.33-550311.7 chandra ccd7 730.5 1181.83 2.98141 1.73205 0.00147506 0.000856935 5.52454 0.999762 0.492 0.492 90 3.01343 F F 4.08e+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