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 X173255.97-301144.9 chandra ccd3 325.167 872.667 5.95076 3.59808 0.00291311 0.00176139 26.8173 1 1.36685 0.794857 114.671 8.63786 5.95076 0 -1 0.866422 A F 6.9e+21 4.6002e-14 1 dx
Report 1 X173218.91-301704.7 chandra ccd1 282.7 64.1001 4.94166 2.23607 0.00241921 0.00109468 12.5886 1 0.492 0.492 116.565 1.91554 F F 6.79e+21 0 1 d
Report srcpi bgdpi arf 2 X173236.12-301158.3 chandra ccd3 848.25 845.75 3.85854 3.17945 0.00188889 0.00155645 10.2589 1 0.589598 0.492 56.9812 6.09112 2 1.85854 -0.0366623 0.839241 F F 6.73e+21 2.70606e-14 1 dx
Report 3 X173244.22-301754.1 chandra ccd3 635.167 122.5 2.98182 1.73205 0.00145971 0.0008479 7.05684 0.999963 0.492 0.492 90 3.67536 F F 7.06e+21 0 1 d
Report srcpi bgdpi arf 1 X173227.59-302326.5 chandra ccd2 882 456 1.91531 2.65831 0.000939054 0.00130334 6.58133 0.999905 0.492 0.492 45 5.69139 1.91531 0 -1 2.01728 F F 7.15e+21 1.4071e-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