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 1 X132249.52+545525.6 xmm mos1 301.788 274.806 29.8994 6.43012 0.381787 0.0821065 8.83724 1 4.83914 4.83914 0 1.71681 F F 1.62126 0 1 dsp
Report srcpi bgdpi 1 X132249.60+545527.1 xmm mos2 301.624 275.072 255.834 19.0305 0.446735 0.033231 0 10.875 10.875 0 1.70966 F F 1.62116 0 1 db
Report srcpi bgdpi 2 X132301.74+545712.1 xmm pn 277.581 299.305 111.068 21.789 0.00555502 0.00108977 2.75932 0.996908 5.92466 5.92466 0 1.4984 F F 1.5854 0 1 ds
Report srcpi bgdpi 3 X132244.67+545654.1 xmm pn 311.396 295.141 195.095 23.5916 0.00975762 0.00117993 4.84684 0.999999 13.5601 4.72935 91.0151 0.990119 A F 1.60219 0 1 ds
Report srcpi bgdpi 4 X132249.50+545527.0 xmm pn 301.829 275.129 16814 144.739 0.84095 0.00723912 417.719 1 5.88252 5.73186 330.102 1.71305 F F 1.62132 0 1 ds

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