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 5 X162912.86-460250.9 chandra ccd2 130.256 501.245 206.825 14.771 0.182219 0.0130137 61.3716 1 1.02133 0.544282 241.669 3.38923 F F 8.15e+21 3.52692e-12 1 dsxf
Report 1 X162929.59-460736.4 chandra ccd1 975.25 778.5 3.97041 2 0.00349794 0.001762 12.7771 1 0.492 0.492 18.0137 2.63889 F F 8.69e+21 0 1 d
Report 1 X162954.87-460258.0 chandra ccd0 275 334.5 1.97493 1.41421 0.00173992 0.00124592 6.07344 0.999818 0.665224 0.492 146.31 7.33309 F F 8.64e+21 0 1 d
Report srcpi bgdpi arf 2 X162928.08-455824.9 chandra ccd0 841.5 890.5 1.95504 1.41422 0.00172239 0.00124592 6.01226 0.999818 0.825109 0.492 116.565 7.99596 A F 8e+21 2.71627e-14 1 dx
Report srcpi bgdpi arf 3 X162922.57-455850.1 chandra ccd0 958.167 839.167 5.92041 2.44949 0.00521589 0.002158 18.2068 1 0.760781 0.492 125.453 7.39991 A F 7.98e+21 8.11874e-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