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 X171809.83-371851.8 chandra ccd7 166.297 755.534 86.6331 10.1619 0.00260377 0.000305418 28.1863 1 0.395712 0.395712 0 0.206607 F F 1.36e+22 3.4349e-14 1 dsx
Report srcpi bgdpi arf 2 X171802.42-372106.5 chandra ccd7 345.278 481.389 7.64306 3.00003 0.000229713 9.01661e-05 2.48669 0.991529 0.492 0.492 158.745 2.87304 F F 1.37e+22 3.1264e-15 1 dx
Report srcpi bgdpi arf 3 X171806.17-371938.5 chandra ccd7 254.997 660.76 8.36734 4.28406 0.000251481 0.000128758 2.72234 0.991529 0.348324 0.348324 0 1.24168 F F 1.36e+22 3.31575e-15 1 dsx
Report srcpi bgdpi arf 4 X171812.10-371854.4 chandra ccd7 111.301 750.255 25.2866 5.74956 0.000759991 0.000172804 8.22706 1 0.393706 0.393706 0 0.487115 F F 1.37e+22 1.04452e-14 1 dsx
Report srcpi bgdpi arf 5 X171759.57-372157.6 chandra ccd7 414.967 377.95 24.3549 5.88762 0.000731989 0.000176953 7.92393 1 1.14016 0.255211 88.3292 3.89806 A F 1.37e+22 1.00192e-14 1 dsx

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