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 X171707.58-371614.2 chandra ccd7 867.433 648.517 19.8249 4.45252 0.014799 0.00332373 34.9619 1 0.89901 0.516637 315.63 3.18153 F F 1.33e+22 2.01232e-13 1 dsx
Report srcpi bgdpi arf 3 X171724.00-371716.1 chandra ccd7 469 522.797 10.3256 3.21335 0.00770786 0.0023987 18.2096 1 0.630714 0.630714 0 2.46854 F F 1.34e+22 1.03348e-13 1 dsx
Report srcpi bgdpi arf 2 X171722.30-371358.8 chandra ccd7 509.833 923.333 5.85862 2.44949 0.00437335 0.0018285 10.3319 1 0.718611 0.50888 136.263 5.23512 F F 1.33e+22 6.07957e-14 1 dx
Report 1 X171715.06-372349.1 chandra ccd6 393.5 698.5 0.990317 1 0.000739252 0.000746481 2.71552 0.991902 0.492 0.492 90 4.79311 F F 1.36e+22 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