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 6 X001137.21+144201.4 chandra ccd7 31.2889 351.246 240.225 15.8965 0.0687503 0.00454944 76.277 1 3.18905 1.97976 2.8028 7.04935 F F 4.1e+20 0 1 ds
Report 1 X001115.23+144601.8 chandra ccd7 679.455 839.824 137.801 12.0484 0.0394375 0.00344816 43.755 1 0.395761 0.395761 0 0.573398 F F 4.16e+20 0 1 ds
Report 1 X001140.28+145436.3 chandra ccd2 1048 723.3 9.13077 3.1623 0.00261305 0.000904986 22.5852 1 2.54631 1.82989 43.6434 10.0653 F F 4.13e+20 0 1 d
Report 1 X001059.74+145601.1 chandra ccd6 845.357 1021.5 5.76805 2.64579 0.00164768 0.000755787 13.4327 1 2.93747 0.804282 136.177 10.1159 A F 4.19e+20 0 1 d
Report 2 X001148.38+145534.0 chandra ccd2 809.5 840.667 4.99952 2.44951 0.00143076 0.000701002 12.3665 1 5.74251 0.972924 35.9783 12.0554 A T 4.12e+20 0 1 d
Report 2 X001102.48+145115.6 chandra ccd6 764.75 441.25 3.96692 2 0.00113318 0.000571314 9.23822 0.999998 0.492 0.492 108.435 5.55923 F T 4.18e+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