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 X061558.24-515424.5 xmm pn 243.042 339.363 37.0841 7.84896 0.0370669 0.00784532 8.35522 1 6.62163 3.73992 83.9473 4.9823 A F 6.32712 1.64068e-13 1 dsx
Report srcpi bgdpi arf 2 X061536.23-515149.2 xmm pn 289.861 375.107 18.3946 6.56435 0.018386 0.0065613 4.14439 0.99992 5.47939 2.51446 350.581 5.59155 F F 6.37453 8.82636e-14 1 dsx
Report srcpi bgdpi arf 3 X061529.54-520459.0 xmm pn 304.084 193.537 11.2056 4.44802 0.0112004 0.00444595 2.52467 0.988849 3.77455 3.77455 0 7.61778 F F 6.43319 9.03691e-14 1 dsx
Report srcpi bgdpi arf 4 X061613.13-515019.7 xmm pn 211.236 395.582 14.548 5.96233 0.0145413 0.00595957 3.27773 0.998835 8.44814 8.44814 0 9.4394 F F 6.27687 7.19692e-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 - 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