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 X154159.79-422933.9 xmm mos2 104.245 279.71 34.3219 14.272 0.00683704 0.00284302 2.63728 0.994672 7.71394 7.71394 0 14.1733 20.7492 18.0369 -0.0699311 0.272395 F F 1.38e+21 2.16539e-13 1 dsx
Report srcpi bgdpi arf 1 X154023.26-422835.2 xmm pn 349.703 293.536 30.5899 11.3546 0.0172818 0.00641481 3.08474 0.998246 6.61469 6.61469 0 3.77695 20.1853 6.74749 -0.498939 0.343578 F F 1.29e+21 8.99358e-14 1 dsx
Report srcpi bgdpi arf 2 X154155.01-422413.1 xmm mos2 116.145 352.317 33.4761 11.4283 0.00666855 0.00227656 3.87781 0.999892 10.875 10.875 0 13.7814 8.96807 21.0975 0.403432 0.398088 F F 1.37e+21 1.98108e-13 1 dpx

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