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 X042439.19+603201.0 chandra ccd7 980.5 670.2 9.85765 3.16228 0.00725587 0.00232764 11.9867 1 0.537089 0.492 127.646 4.34308 F F 3.39e+21 6.10159e-14 1 dx
Report 1 X042556.31+604005.4 chandra ccd6 262.75 653.25 3.87712 2 0.00285381 0.00147213 14.5267 0.999999 1.06498 0.694788 80.0724 8.24675 A F 3.35e+21 0 1 d
Report 2 X042518.68+603601.5 chandra ccd6 824.5 156.5 0.99781 1 0.000734453 0.000736065 3.73856 0.99758 0.492 0.492 90 2.20268 F F 3.37e+21 0 1 d
Report 3 X042531.20+603606.5 chandra ccd6 637.167 166.833 2.97179 1.73205 0.00218743 0.0012749 11.1346 0.999999 0.492 0.492 160.097 3.27267 F F 3.36e+21 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