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 1 X125632.78+215934.5 xmm mos1 403.274 287.124 132.195 18.9954 0.0166963 0.00239913 0 10.875 10.875 0 7.64483 U U 2.66e+20 d
Report 1 X125632.77+215938.3 xmm mos2 403.31 287.961 135.064 18.6892 0.0163486 0.00226221 0 10.875 10.875 0 7.64114 U U 2.66e+20 d
Report 3 X125658.86+215341.8 xmm mos2 319.9 206.095 100.835 16.8155 0.0135313 0.00225651 0 10.875 10.875 0 6.87325 U U 2.67e+20 d
Report 2 X125710.08+215352.8 xmm mos2 284.011 209.064 96.5289 16.8828 0.0133539 0.00233559 0 10.875 10.875 0 6.56336 U U 2.66e+20 d
Report 2 X125658.97+215344.9 xmm mos1 319.553 206.55 74.3581 15.7811 0.0108527 0.00230329 0 10.875 10.875 0 6.83542 U U 2.67e+20 d

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