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 X111816.96+074558.7 chandra ccd7 213.229 776.925 404.532 23.4223 0.0276299 0.00159976 47.6625 1 0.487349 0.487349 0 0.283732 F F 3.57e+20 2.29824e-13 1 dsxf
Report srcpi bgdpi arf 5 X111816.15+074316.2 chandra ccd7 237.679 446.524 40.982 6.40172 0.00279911 0.000437244 4.82855 0.999997 0.848027 0.416453 105.264 2.9989 F F 3.6e+20 4.11253e-14 1 dsx
Report srcpi bgdpi arf 1 X111837.57+073914.9 chandra ccd3 912.635 517.195 11.8705 7.29514 0.000810769 0.000498266 1.84603 0.966509 2.4918 2.4918 0 8.71911 F F 3.73e+20 1.09359e-14 1 dsx
Report srcpi bgdpi arf 2 X111836.73+073952.1 chandra ccd3 937.281 592.281 27.4648 5.65692 0.00187587 0.000386372 4.27117 0.999947 1.87286 1.5609 37.4005 8.0862 F T 3.71e+20 3.05565e-14 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 - 7.99 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), T = 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