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 1 X183216.23-102302.5 xmm mos2 110.814 300.953 145.834 15.3916 0.030346 0.00320277 15.282 1 9.00564 3.90376 91.8085 13.6207 54.9648 92.215 0.253093 0.0937007 A T 1.39e+22 1.93159e-12 1 dsx
Report srcpi bgdpi arf 2 X183216.21-102300.1 xmm mos1 110.866 301.506 91.1994 12.6756 0.0189565 0.00263472 13.2457 1 6.71888 3.27886 85.4469 13.6063 34.4052 64.2239 0.302331 0.118612 F T 1.39e+22 1.57414e-12 1 dsx
Report srcpi bgdpi arf 1 X183035.72-102104.4 xmm pn 451.722 328.119 29.8113 12.3187 0.0109874 0.00454023 2.69966 0.995243 11.1137 3.02549 81.4177 11.3468 23.9 -1.20076 -1 0.409238 A T 1.49e+22 2.96034e-13 1 dsx
Report srcpi bgdpi arf 1 X183156.16-102447.2 xmm mos1 178.895 276.912 21.6629 6.85596 0.0045028 0.00142506 3.1463 0.99874 9.59281 3.64443 111.419 8.83051 4.37103 12.5106 0.482157 0.387927 F T 1.42e+22 1.60086e-13 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 - 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