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 2 X105120.80+324555.5 chandra ccd7 559.812 554.919 16.865 4.1067 0.0097231 0.00236762 29.921 1 0.670521 0.670521 0 2.18227 F F 2e+20 0 1 ds
Report 1 X105137.23+324402.5 chandra ccd7 137.833 324.833 5.89175 2.44949 0.00339669 0.00141217 10.4528 1 0.707623 0.492 138.716 3.98539 F F 2.01e+20 0 1 d
Report 3 X105116.81+324315.4 chandra ccd7 661.75 229 3.95394 2 0.00227951 0.00115303 7.01487 0.999979 0.492 0.492 78.0188 0.63467 F F 2.02e+20 0 1 d
Report 1 X105043.55+324736.1 chandra ccd3 204 289.5 3.83027 2.00001 0.00220822 0.00115304 10.8615 0.999991 0.829775 0.492 65.9936 8.23565 A F 2e+20 0 1 d
Report 2 X105038.63+324925.9 chandra ccd3 329.75 512.75 3.7015 2.00001 0.00213398 0.00115304 10.4963 0.999991 1.14287 0.806944 57.2836 10.061 F F 2e+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