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 X174328.65-321357.1 chandra ccd0 241.1 29.7 4.95261 3.39792 0.00254523 0.00174625 22.7511 1 0.879452 0.492 153.863 8.64155 2.95261 2 -0.192345 0.709266 A F 7.78e+21 4.98744e-14 1 dx
Report 2 X174405.58-320718.7 chandra ccd2 348 971.25 3.94933 2 0.00202963 0.00102783 10.6891 1 0.492 0.492 142.018 4.91771 F F 7.76e+21 0 1 d
Report srcpi bgdpi arf 1 X174341.41-321406.3 chandra ccd2 972 143 3.77123 3.17945 0.0019381 0.00163397 7.88459 0.999996 0.729085 0.492 123.401 8.22662 1 2.77123 0.469668 0.948025 F F 7.71e+21 3.15685e-14 1 dx
Report 3 X174353.43-320954.2 chandra ccd2 661.833 655.5 2.97146 1.73205 0.00152708 0.000890131 8.04243 0.999987 0.492 0.492 180 4.54562 F F 7.76e+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