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 X100129.01-593939.9 chandra ccd7 618.136 614.136 11.9263 3.45345 0.000691773 0.000200314 7.52935 1 0.587512 0.587512 0 0.409963 0 12.9153 1 0.519206 F F 8.08e+21 1.03858e-14 1 dsx
Report srcpi bgdpi arf 2 X100156.37-594317.9 chandra ccd7 197.551 170.614 8.2001 4.01322 0.000475637 0.000232782 5.17691 0.999936 1.79677 0.340481 246.375 5.12759 6.51866 -0.80224 -1 0.830572 F F 7.9e+21 5.55971e-15 1 dsx
Report srcpi bgdpi arf 3 X100137.30-594032.8 chandra ccd7 490.471 506.504 66.6853 8.16611 0.003868 0.000473665 42.1 1 0.448207 0.448207 0 1.48272 29.8306 36.8306 0.105009 0.139467 F F 8.04e+21 4.30609e-14 1 dsx

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