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 X061536.62+710212.6 xmm pn 307.137 318.813 194.471 19.1949 0.32483 0.0320617 15.6302 1 7.12692 7.12692 0 1.62036 F T 2.71885 1.20246e-12 1 dsxf
Report srcpi bgdpi arf rmf 1 X061536.37+710213.6 xmm mos1 307.414 319.037 150.666 15.9499 0.169632 0.0179577 20.8988 1 5.53457 5.53457 0 1.63632 F T 2.71836 2.84828e-12 1 dsxf
Report srcpi bgdpi arf rmf 1 X061536.46+710213.1 xmm mos2 307.311 318.913 409.883 22.0918 0.187608 0.0101117 54.1334 1 7.14011 5.45671 359.98 1.62886 F T 2.71831 3.1522e-12 1 dsxf
Report srcpi bgdpi arf 2 X061343.88+710726.0 xmm mos1 432.867 391.408 26.9103 7.61363 0.0302979 0.00857207 3.73272 0.999709 6.17504 3.57443 206.914 11.8737 F T 2.60014 6.86582e-13 1 dsx
Report srcpi bgdpi arf 2 X061343.20+710725.7 xmm mos2 433.627 391.35 87.0064 11.1132 0.0398239 0.00508666 11.491 1 6.27865 3.77043 52.5899 11.8916 F T 2.59947 1.18806e-12 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