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 X162722.33+550106.5 chandra ccd7 463.095 779.976 29.0316 6.4809 0.0201066 0.00448853 66.1995 1 8.38824 4.16726 171.96 13.1367 A F 1.39e+20 0 1 d
Report 1 X162604.24+551843.7 chandra ccd0 801.5 580.853 15.5268 4.12313 0.0107535 0.00285559 54.5559 1 2.2819 2.00871 43.0179 8.84989 F F 1.36e+20 0 1 d
Report 1 X162637.97+551101.0 chandra ccd2 308.071 669.214 6.96292 2.64575 0.00482236 0.00183239 24.9508 1 0.739506 0.492 7.25553 3.60231 A F 1.36e+20 0 1 d
Report 1 X162746.41+551915.5 chandra ccd1 92.8999 594.5 4.73744 2.23608 0.00328104 0.00154866 17.193 1 1.5357 0.748944 45.3472 9.20097 A F 1.41e+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