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 rmf 1 X163226.35+823221.1 chandra ccd7 302.115 192.626 119.7 15.9732 0.00263425 0.000351523 4.76441 0.999998 1.5 1.5 0 0.746765 T F 5.57e+20 1.46064e-14 1 dscxf
Report srcpi bgdpi arf rmf 2 X163224.07+823222.9 chandra ccd7 311.107 196.318 216.613 17.6112 0.00476703 0.000387572 8.62183 1 1.73512 1.73512 0 0.835502 T F 5.57e+20 3.29807e-14 1 dscx
Report srcpi bgdpi arf 3 X163222.10+823224.1 chandra ccd7 318.91 198.91 88.8213 11.3703 0.0019547 0.000250228 3.53535 0.999751 1.5 1.5 0 0.954238 T F 5.57e+20 1.35332e-14 1 dscx
Report srcpi bgdpi arf rmf 4 X163231.83+823216.3 chandra ccd7 280.409 182.891 31175.4 182.841 0.686081 0.0040238 1240.87 1 0.418631 0.418631 0 0.574935 F T 5.57e+20 4.72323e-12 1 dsx

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