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 X152553.69+513648.1 xmm pn 310.159 278.21 519.268 33.0776 0.05481 0.00349142 0 10.875 10.875 0 1.69492 F F 2.11437 1.3136e-13 1 dbx
Report srcpi bgdpi arf 1 X152553.88+513648.7 xmm mos2 309.767 278.42 85.4994 14.1736 0.0154931 0.00256836 7.95931 1 5.75534 3.35635 298.534 1.65336 F F 2.11386 1.94885e-13 1 dsx
Report srcpi bgdpi arf 1 X152553.88+513647.5 xmm mos1 309.771 278.139 91.0771 13.8859 0.015938 0.00242994 10.1555 1 5.84599 5.84599 0 1.68873 F F 2.11404 1.77595e-13 1 dsx
Report srcpi bgdpi arf 2 X152631.04+514429.4 xmm mos1 230.381 384.38 22.2352 9.01966 0.00389103 0.00157839 2.47932 0.991284 5.85182 5.85182 0 7.90142 F F 1.97357 9.38439e-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