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 3 X160843.90+071508.2 chandra ccd7 915.5 909 5.91531 3.59808 0.00379934 0.00231101 20.326 1 0.492 0.492 113.745 0.187393 4 1.91531 -0.352424 0.65348 F F 3.98e+20 2.84993e-14 1 dx
Report srcpi bgdpi arf 2 X160842.79+071108.9 chandra ccd7 949 422.5 3.92263 3.17945 0.00251946 0.00204213 14.1021 1 0.539213 0.492 49.7312 3.95753 3 -0.0773723 -1 1.41421 F F 4.03e+20 2.19169e-14 1 dx
Report srcpi bgdpi arf 1 X160901.56+071041.7 chandra ccd7 381.25 367.25 3.94014 3.17945 0.00253071 0.00204213 16.1045 1 0.696119 0.492 58.7764 6.34717 4 0 -1 1.14412 F F 4.05e+20 2.0678e-14 1 dx
Report 4 X160847.91+071338.0 chandra ccd7 794.167 725.5 2.98799 1.73205 0.00191916 0.00111248 6.80735 0.999951 0.492 0.492 5.35186e-08 1.88615 F F 4e+20 0 1 d
Report srcpi bgdpi arf 1 X160810.73+072115.4 chandra ccd6 1072.5 974.5 0.915307 2.32288 0.000587907 0.001492 3.14516 0.99661 0.492 0.492 90 10.125 -0.0846933 1 1 3.41421 F F 3.87e+20 1.36661e-14 1 dx

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