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 1 X115611.03-630834.1 xmm pn 295.328 303.049 184.924 22.7205 0.0510463 0.00627178 0 10.875 10.875 0 0.403244 U U 1.39e+22 d
Report 2 X115607.42-630855.8 xmm pn 300.953 298.08 214.168 24.3394 0.0589217 0.00669624 0 10.875 10.875 0 0.184266 U U 1.39e+22 d
Report 3 X115451.04-631331.1 xmm pn 419.592 234.535 183.755 18.9135 0.0420691 0.00433008 0 10.875 10.875 0 9.93061 U U 1.38e+22 d
Report 4 X115618.90-630718.1 xmm pn 283.064 319.645 84.8398 15.3603 0.0272146 0.00492722 0 10.875 10.875 0 1.89908 U U 1.39e+22 d
Report 5 X115614.87-630743.4 xmm pn 289.343 314.911 118.12 19.7679 0.0330136 0.00552497 0 10.875 10.875 0 1.36425 U U 1.39e+22 d
Report 6 X115614.07-630812.9 xmm pn 290.602 307.998 134.591 20.8741 0.0376765 0.00584335 0 10.875 10.875 0 0.89623 U U 1.39e+22 d
Report 7 X115619.24-630652.0 xmm pn 282.532 328.855 100.851 15.1877 0.0409785 0.00617121 0 10.875 10.875 0 2.48858 U U 1.39e+22 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 - 10.00 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), A = 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