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 X032613.95+022515.2 xmm pn 316.125 315.073 7040.5 93.2942 1.46469 0.0194087 172.631 1 5.87538 5.87538 0 1.76711 F T 2.43117 0 1 ds
Report srcpi bgdpi 1 X032613.89+022514.5 xmm mos2 316.325 314.948 4723.97 81.5234 0.859262 0.0148286 1082.87 1 10.875 10.875 0 1.76491 F T 2.43145 0 1 d
Report srcpi bgdpi 1 X032613.90+022514.8 xmm mos1 316.285 314.993 3004.81 62.3699 0.539657 0.0112015 100.994 1 5.39893 5.39893 0 1.77265 F T 2.43147 0 1 ds
Report srcpi bgdpi 2 X032610.77+021336.9 xmm mos2 327.068 154.546 25.7112 6.68897 0.00467137 0.00121529 5.89373 1 7.64708 3.77269 8.43414 10.6407 F F 2.56874 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