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 8 X113151.60-123158.5 chandra ccd7 199.043 648.885 16192.9 131.239 0.632041 0.00512251 713.299 1 0.631737 0.364319 81.6316 0.319483 A F 3.42e+20 5.50592e-12 1 dscxf
Report srcpi bgdpi arf rmf 1 X113151.51-123158.4 chandra ccd7 201.722 649.105 21659.1 147.17 0.845397 0.00574435 954.086 1 1.225 1.225 0 0.318166 T F 3.42e+20 6.27802e-12 1 dscx
Report srcpi bgdpi arf rmf 1 X113243.45-123629.3 chandra ccd2 280.337 301.881 300.641 19.7595 0.0117346 0.000771251 31.7263 1 8.73447 7.02995 318.435 13.4835 F F 3.48e+20 1.88033e-13 1 dsxf
Report srcpi bgdpi arf 1 X113200.87-122929.6 chandra ccd6 605.046 161.643 27.9281 5.2847 0.00109009 0.000206272 19.4937 1 0.715342 0.715342 0 3.0998 F F 3.4e+20 1.15066e-14 1 dsx
Report srcpi bgdpi arf 1 X113206.48-123956.9 chandra ccd3 668.928 650.986 23.5245 5.91622 0.000918205 0.000230921 18.065 1 3.09965 2.86481 138.978 9.03185 F F 3.48e+20 1.24575e-14 1 dx

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