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 X174502.77-315933.9 chandra ccd0 678.846 650.729 39.4869 6.28386 0.0202933 0.00322943 103.679 1 2.76773 1.78529 29.5358 6.74421 27.7269 14.6723 -0.307898 0.188373 F F 7.55e+21 3.12936e-13 1 dsx
Report srcpi bgdpi arf 3 X174426.09-321011.4 chandra ccd3 719.722 525.389 8.85063 4.1225 0.00454849 0.00211862 22.9004 1 1.33462 0.784784 58.6522 6.53239 0.95021 7.90042 0.785279 0.597952 A F 7.51e+21 6.94191e-14 1 dx
Report srcpi bgdpi arf 1 X174513.80-320747.9 chandra ccd1 530.072 687.928 6.79345 3.78388 0.00349127 0.0019446 14.9478 1 1.00892 0.492 31.8793 6.05002 5.91738 0.876069 -0.742084 0.701766 A F 7.18e+21 5.11058e-14 1 dx
Report srcpi bgdpi arf 4 X174509.74-320741.6 chandra ccd1 634.833 700.833 5.93065 3.59808 0.00304786 0.00184911 22.521 1 0.600674 0.492 168.019 5.22167 4.93065 1 -0.662769 0.737487 F F 7.22e+21 4.46053e-14 1 dx
Report srcpi bgdpi arf 2 X174451.41-321210.6 chandra ccd3 66.3333 283.333 5.94374 3.59808 0.00305459 0.00184911 25.0598 1 1.25267 0.832221 160.477 6.75751 0 5.94374 1 0.867445 A F 7.23e+21 4.51151e-14 1 dx
Report srcpi bgdpi arf 2 X174513.45-321021.3 chandra ccd1 539.5 376.1 4.83583 3.39792 0.00248522 0.00174625 11.9352 1 0.952182 0.615394 124.099 7.3618 1.89056 2.94528 0.218106 0.730088 A F 7.1e+21 4.32619e-14 1 dx
Report srcpi bgdpi arf 3 X174521.73-320937.5 chandra ccd1 325.75 464.75 3.96836 3.17945 0.00203941 0.00163397 22.3093 1 2.07033 0.773647 170.155 8.36629 4 -0.031641 -1 1.14412 A F 7.05e+21 3.16186e-14 1 dx
Report 1 X174450.16-320949.9 chandra ccd3 98.5 569.167 2.98564 1.73205 0.00153437 0.000890131 7.82152 0.999983 0.550073 0.492 18.4349 4.39918 F F 7.32e+21 0 1 d
Report 1 X174443.94-320157.9 chandra ccd2 145.167 502.5 2.96843 1.73205 0.00152553 0.000890131 8.36833 0.999991 0.492 0.492 139.731 3.58262 F F 7.67e+21 0 1 d
Report 5 X174512.11-320931.4 chandra ccd1 573.833 477.5 2.92187 1.73205 0.0015016 0.000890132 7.85877 0.999986 0.510281 0.492 28.155 6.61365 F F 7.13e+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