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 X165749.67+352031.8 xmm pn 292.77 272.162 3605.24 67.999 4.44778 0.0838903 112.96 1 6.10677 6.10677 0 1.95569 F T 7.52315 2.08808e-11 1 dsxf
Report srcpi bgdpi arf 1 X165749.74+352032.5 xmm mos2 292.589 272.177 400.982 23.7916 2.4212 0.143658 0 10.875 10.875 0 1.95047 F T 7.52299 2.36528e-11 1 dbx
Report srcpi bgdpi arf rmf 4 X165749.71+352032.0 xmm mos1 292.683 272.202 2891.75 61.4529 1.63846 0.0348191 97.2214 1 5.58218 5.58218 0 1.9563 F T 7.523 2.53421e-11 1 dscxf
Report srcpi bgdpi arf 3 X165741.67+352232.7 xmm pn 315.285 300.235 85.0906 13.5908 0.0281384 0.00449432 2.66608 0.995713 10.875 10.875 0 1.22844 T T 7.5554 1.17116e-13 1 dbpx
Report srcpi bgdpi arf 4 X165800.53+352333.2 xmm pn 262.248 313.856 92.0179 15.169 0.0265096 0.00437004 2.88313 0.997758 10.875 10.875 0 2.85193 F T 7.49482 7.77371e-14 1 dbx
Report srcpi bgdpi arf 3 X165748.54+351939.7 xmm mos1 295.961 261.451 50.3992 13.2636 0.0102147 0.00268819 1.69443 0.955189 21.75 21.75 0 2.68744 T T 7.52466 9.89161e-14 1 dbcx

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