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 1 X162021.82+173624.0 chandra ccd7 290.299 315.875 7120.18 86.5876 0.245698 0.0029879 366.597 1 0.418308 0.39321 312 0.589915 F T 4.05e+20 0 1 ds
Report 1 X162010.51+172058.3 chandra ccd5 185.012 473.774 353.133 39.4106 0.0108762 0.00121382 10.7256 1 5.70894 5.10607 132.635 15.0841 F T 4.15e+20 0 1 d
Report 2 X162011.28+172427.6 chandra ccd5 162.836 899.755 22694.6 154.203 0.763769 0.00518959 689.296 1 7.76633 6.0419 21.7996 11.6192 F F 4.13e+20 0 1 ds
Report 3 X162015.85+172644.2 chandra ccd6 243.069 161.305 18.8429 7.84596 0.000580346 0.000241649 2.88305 0.996722 1.65197 1.65197 0 9.16667 F F 4.12e+20 0 1 ds
Report 2 X162012.61+172832.4 chandra ccd6 336.695 380.817 22.4248 6.4033 0.000690667 0.000197217 3.43109 0.99943 3.35216 1.92491 7.55168 7.57384 A F 4.1e+20 0 1 db
Report 1 X162015.65+172830.7 chandra ccd6 248.269 377.269 19.9034 5.09909 0.000613008 0.000157048 3.0453 0.997837 1.70471 1.11248 131.937 7.44505 A T 4.11e+20 0 1 d

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