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 1 X061536.46+710214.6 xmm pn 316.262 313.264 97.404 14.4974 0.33245 0.049481 9.17234 1 5.57911 3.69893 10.2678 1.69598 F F 2.71844 1.1117e-12 1 dbsx
Report srcpi bgdpi arf rmf 2 X061536.46+710214.1 xmm mos2 316.259 313.158 324.987 23.247 0.162366 0.0116144 25.1793 1 6.45962 4.9288 10.1941 1.6875 F T 2.71857 2.62382e-12 1 dsxf
Report srcpi bgdpi arf rmf 2 X061536.30+710214.3 xmm mos1 316.448 313.212 322.108 24.3004 0.155689 0.0117454 24.2928 1 5.23717 5.23717 0 1.69667 F T 2.71838 2.28175e-12 1 dsxf
Report srcpi bgdpi arf 1 X061343.42+710727.9 xmm mos1 442.285 385.92 74.5004 15.9152 0.0360093 0.00769251 5.61869 1 7.37363 4.60964 56.2812 12.2239 F F 2.59964 7.53059e-13 1 dsx
Report srcpi bgdpi arf 1 X061343.24+710726.3 xmm mos2 442.488 385.702 162.015 16.9234 0.041625 0.00434796 12.5526 1 10.875 10.875 0 12.2106 F F 2.5997 9.16712e-13 1 dx

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