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 X172320.81+341757.8 xmm pn 290.147 276.348 1813.45 47.4174 4.25045 0.111139 86.952 1 6.16789 6.16789 0 1.72015 F T 2.18408 9.19268e-12 1 dbsxf
Report srcpi bgdpi arf rmf 1 X172320.86+341757.7 xmm mos1 290.007 276.323 2882.23 60.8923 1.32078 0.0279039 139.104 1 5.53297 5.53297 0 1.7259 F T 2.18388 1.19702e-11 1 dsxf
Report srcpi bgdpi arf rmf 1 X172320.85+341758.3 xmm mos2 290.023 276.456 6433.96 90.9575 1.11626 0.0157807 209.587 1 5.81654 5.30046 -0 1.72105 F T 2.18389 1.41248e-11 1 dsxf
Report srcpi bgdpi arf 3 X172323.91+341613.2 xmm mos1 281.318 252.298 84.6516 10.8467 0.0387916 0.00497051 4.08549 0.999961 14.8927 14.8927 0 3.1332 T F 2.17129 3.7499e-13 1 dsx
Report srcpi bgdpi arf 4 X172321.88+341848.3 xmm mos2 287.107 286.935 63.1764 13.5433 0.00982375 0.00210595 2.05798 0.979283 10.875 10.875 0 1.17051 T T 2.18359 1.22339e-13 1 dbx

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