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 X162344.12+263244.4 xmm mos1 263.611 255.221 70.7862 10.9824 0.0117155 0.00181765 0 10.875 10.875 0 4.02391 U U 3.14e+20 d
Report 3 X162344.06+263245.4 xmm mos2 263.784 255.738 61.5406 10.6129 0.0104848 0.00180815 0 10.875 10.875 0 3.98688 U U 3.14e+20 d
Report 2 X162335.27+263413.6 xmm mos1 290.895 276.034 46.5891 10.1158 0.00737288 0.00160086 0 10.875 10.875 0 1.71377 U U 3.12e+20 d
Report 1 X162334.34+263430.7 xmm mos2 293.775 279.918 43.3774 9.74051 0.00688456 0.00154595 0 10.875 10.875 0 1.38453 U U 3.12e+20 d
Report 2 X162335.72+263405.9 xmm mos2 289.532 274.899 33.5161 8.46047 0.00543728 0.00137253 0 10.875 10.875 0 1.82454 U U 3.13e+20 d
Report 3 X162334.48+263347.3 xmm mos1 293.34 270.032 28.4385 8.21096 0.00452488 0.00130645 0 10.875 10.875 0 2.09224 U U 3.13e+20 d
Report 4 X162354.04+263937.8 xmm mos1 233.084 350.531 37.3098 8.18128 0.00855242 0.00187537 0 10.875 10.875 0 6.05917 U U 3.09e+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