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 1 X163946.07+282421.6 chandra ccd6 316.183 670.092 19.3258 4.39611 0.0125332 0.00285097 64.9196 1 3.56307 3.56307 0 8.03036 18.746 0.576646 -0.940314 0.39658 F F 3.28e+20 1.60527e-13 1 dsx
Report 4 X163909.11+282447.1 chandra ccd7 291.667 502.833 5.96825 2.44949 0.0038705 0.00158853 13.6953 1 0.492 0.492 101.153 0.181602 F F 3.24e+20 0 1 d
Report srcpi bgdpi arf 1 X163906.29+282046.7 chandra ccd7 367.5 14.25 4.80883 3.39792 0.0031186 0.0022036 10.9985 1 0.653886 0.492 52.6881 4.21824 2.80883 2 -0.168198 0.727399 F F 3.33e+20 4.80438e-14 1 dx
Report srcpi bgdpi arf 3 X163853.07+282709.3 chandra ccd7 721.833 791.833 2.91531 2.93649 0.00189062 0.00190436 10.0175 0.999998 0.492 0.492 45 4.25652 2 0.915307 -0.372068 1.09797 F F 3.17e+20 1.47475e-14 1 dx
Report srcpi bgdpi arf 2 X163846.45+282849.1 chandra ccd7 899 995 1.94674 2.65831 0.00126249 0.00172395 8.43551 0.999976 0.782767 0.492 45 6.39955 1.94674 0 -1 1.9847 A F 3.12e+20 1.06468e-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