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 X174718.23-304110.7 chandra ccd3 643.254 1041.03 40.5249 6.36592 0.0188149 0.00295556 99.0377 1 1.70416 1.09359 90.0397 4.99618 F F 8.87e+21 2.92022e-13 1 dsx
Report srcpi bgdpi arf 2 X174758.57-305020.6 chandra ccd1 616.864 105.955 10.501 3.31664 0.00487536 0.00153984 24.711 1 1.79128 1.6429 104.245 9.4587 F F 8.34e+21 8.9869e-14 1 dx
Report srcpi bgdpi arf 1 X174750.95-304908.8 chandra ccd1 816.072 251.928 6.63892 2.64576 0.0030823 0.00122837 15.6228 1 1.07921 0.981762 82.7896 7.7885 F F 8.4e+21 4.99494e-14 1 dx
Report 2 X174734.19-304605.0 chandra ccd3 224 442.5 3.96009 2 0.00183858 0.000928555 9.67796 0.999999 0.492 0.492 180 4.70804 F F 8.51e+21 0 1 d
Report srcpi bgdpi arf 1 X174754.88-303445.7 chandra ccd0 898.5 983.167 2.86137 1.73205 0.00132847 0.000804154 6.78225 0.999964 0.96471 0.492 39.1159 7.46242 A F 8.68e+21 2.11878e-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