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 X125732.13+241238.0 xmm pn 301.061 321.254 1653.39 55.6299 2.41317 0.0811934 43.551 1 5.64581 5.64581 0 1.66029 1330.85 412.479 -0.526792 0.0326542 F F 1.25e+20 6.29727e-12 1 dsx
Report srcpi bgdpi arf 1 X125732.03+241238.3 xmm mos2 301.37 321.145 652.213 30.4406 0.974012 0.0454599 44.6065 1 10.875 10.875 0 1.66 457.459 122.248 -0.578243 0.0576441 F F 1.25e+20 1.09751e-11 1 dbx
Report srcpi bgdpi arf rmf 1 X125732.13+241238.7 xmm mos1 301.05 321.435 492.421 28.0176 0.856202 0.0487159 28.7889 1 5.63058 5.63058 0 1.66686 359.995 103.2 -0.5544 0.0577762 F F 1.25e+20 1.0197e-11 1 dbsx

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