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 X002403.52-720452.0 chandra ccd3 212.519 855.973 76.736 9.0637 0.0907986 0.0107247 50.545 1 0.380109 0.380109 0 0.851065 F F 5.42e+20 8.5315e-13 1 dsx
Report srcpi bgdpi arf 2 X002400.97-720453.1 chandra ccd3 236.441 853.588 48.8701 6.99072 0.057826 0.00827183 32.1901 1 0.432478 0.432478 0 0.713093 F F 5.41e+20 5.43526e-13 1 dsx
Report srcpi bgdpi arf 3 X002404.30-720457.9 chandra ccd3 205.295 843.824 47.6164 7.13751 0.0563426 0.00844553 31.3643 1 0.398476 0.398476 0 0.956887 F F 5.42e+20 5.30048e-13 1 dsx
Report 4 X002402.18-720541.9 chandra ccd3 225.186 754.505 13.3693 3.72108 0.0158193 0.004403 8.80618 1 0.363836 0.363836 0 1.44601 F F 5.45e+20 0 1 ds
Report 5 X002411.09-720620.0 chandra ccd3 141.25 676.5 3.99725 2 0.00472974 0.0023665 2.63294 0.990538 0.492 0.492 147.312 2.33578 F F 5.49e+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