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 X042002.04-502248.3 xmm pn 298.064 321.936 161.633 36.6756 0.0187615 0.00425711 4.69842 0.999998 3.88206 3.88206 0 1.70784 28.6566 7.28171 -0.594766 0.38997 F T 1.66e+20 6.82575e-14 1 dsx
Report srcpi bgdpi arf 1 X042001.86-502249.1 xmm mos1 298.453 321.743 23.8748 9.86529 0.00509364 0.00210474 2.78578 0.996422 6.98202 2.74317 132.301 1.66865 4.81579 1.18166 -0.605945 0.870319 F T 1.66e+20 7.92041e-14 1 dbsx
Report srcpi bgdpi arf 1 X042002.11-502247.8 xmm mos2 297.909 322.038 23.2437 8.24932 0.00487867 0.00173147 3.4724 0.999524 4.37569 4.37569 0 1.71371 5.68666 -1.5855 -1 1.03512 F T 1.66e+20 7.19526e-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