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 X161729.15-510200.1 chandra ccd3 254.847 457.531 73.6684 14.651 0.0200272 0.00398296 4.59545 0.999995 3.76062 3.76062 0 6.47779 T F 2.07e+22 0 1 ds
Report 3 X161725.78-510354.1 chandra ccd3 319.444 225.754 140.229 18.86 0.0381222 0.0051272 8.74751 1 6.00951 6.00951 0 8.24535 T F 2.07e+22 0 1 ds
Report 6 X161734.47-510317.4 chandra ccd3 152.963 300.479 50.3415 16.2939 0.0136857 0.0044296 3.14031 0.998914 3.87707 3.87707 0 7.86493 F F 2.07e+22 0 1 ds
Report 8 X161724.80-510224.3 chandra ccd3 338.252 408.293 29.7129 14.5275 0.00807765 0.0039494 1.8535 0.965448 2.50598 2.50598 0 6.8104 F F 2.07e+22 0 1 ds
Report 9 X161736.20-510224.9 chandra ccd3 119.636 407.12 3728.52 65.2725 1.01362 0.0177448 232.586 1 2.60553 1.59713 345.361 7.06927 A T 2.07e+22 0 1 ds

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