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 X174554.04-311500.5 chandra ccd7 598.417 937.026 65.6178 11.533 0.0304649 0.00535453 115.17 1 10.9557 6.89228 101.635 15.3681 A F 8.46e+21 4.87704e-13 1 dx
Report srcpi bgdpi arf 2 X174633.14-312213.9 chandra ccd3 881.542 468.545 16.175 4.69908 0.00750979 0.00218171 6.65554 1 1.53472 1.53472 0 8.0759 F F 8.02e+21 1.20209e-13 1 dsx
Report 2 X174654.61-311549.6 chandra ccd2 507.5 207.643 6.98455 2.64575 0.00324277 0.00122836 16.5082 1 0.492 0.492 180 2.93222 F F 7.99e+21 0 1 d
Report 1 X174657.94-312035.4 chandra ccd3 235.7 668.7 4.95258 2.23607 0.00229937 0.00103816 2.03784 0.961126 0.597601 0.492 80.1006 3.148 F F 7.8e+21 0 1 d
Report 1 X174653.30-311502.9 chandra ccd2 541.833 302.5 2.96507 1.73205 0.00137662 0.000804152 7.00802 0.999963 0.54799 0.492 146.981 3.68418 F F 8.03e+21 0 1 d
Report 1 X174732.89-311217.4 chandra ccd0 497.5 821.5 1.97037 1.41421 0.000914797 0.000656588 5.16364 0.999539 0.521845 0.492 45 8.15451 F F 7.77e+21 0 1 d
Report 2 X174719.02-311540.3 chandra ccd0 859.25 409.5 3.97091 2 0.00184361 0.000928555 10.4064 1 0.492 0.492 90 3.71758 F F 7.78e+21 0 1 d

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