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 1 X161734.32-510304.8 chandra ccd3 995.231 52.5698 46.6691 11.5733 0.0094702 0.00234848 3.67628 0.999773 3.70387 3.70387 0 6.42574 T F 2.07e+22 1.85846e-13 1 dsx
Report srcpi bgdpi arf 4 X161811.42-510236.2 chandra ccd3 283.577 109.731 23.6367 6.40332 0.00479641 0.00129938 1.86194 0.964847 1.57789 1.16473 165.496 8.52351 F F 2.04e+22 1.01187e-13 1 dx
Report srcpi bgdpi arf 7 X161741.92-510130.2 chandra ccd3 849.569 244.843 27.1254 12.7924 0.00550435 0.00259587 2.13676 0.982567 2.43244 2.20837 0 7.97457 F F 2.07e+22 1.13097e-13 1 dsx
Report srcpi bgdpi arf rmf 9 X161736.26-510224.7 chandra ccd3 958.161 134.163 1282.56 39.2712 0.26026 0.00796901 101.031 1 2.02487 2.02487 0 7.05476 F F 2.07e+22 2.92594e-12 1 dsxf

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