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 X110109.63+285531.9 xmm pn 157.84 280.703 119.531 19.9244 0.0248876 0.00414847 6.81441 1 8.4094 4.33388 77.3298 10.2821 A F 5.65238 1.77582e-13 1 dsxf
Report srcpi bgdpi arf 2 X110022.33+285817.9 xmm pn 300.618 318.753 71.3439 24.4869 0.0148546 0.00509845 4.06729 0.999962 4.29825 4.29825 0 1.49217 F F 5.48181 5.11442e-14 1 dsx
Report srcpi bgdpi arf 1 X110109.51+285523.8 xmm mos2 158.212 278.839 12.9769 6.38892 0.00771815 0.00379988 2.57639 0.992873 5.61464 5.61464 0 10.2732 F F 5.65184 2.4048e-13 1 dsx
Report srcpi bgdpi arf 4 X105958.72+285850.6 xmm pn 371.837 326.311 59.1208 18.6765 0.0123096 0.00388866 3.37045 0.999449 5.43022 5.43022 0 5.70172 F F 5.39609 4.6499e-14 1 dsx
Report srcpi bgdpi arf 5 X110023.66+284953.8 xmm pn 296.602 202.863 42.054 18.355 0.0087561 0.00382171 2.39748 0.990412 3.49873 3.49873 0 6.92335 F F 5.4806 7.91524e-14 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