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 X101953.40-141434.6 chandra ccd6 871.7 938.9 4.8317 3.39792 0.00471417 0.00331526 11.7775 1 0.49575 0.492 31.7175 3.06178 4 0.831697 -0.655733 0.853731 F F 6.92e+20 5.0217e-14 1 dx
Report srcpi bgdpi arf 1 X101949.97-140445.9 chandra ccd7 488.1 1202.5 4.82058 3.39792 0.00470333 0.00331526 11.3807 1 0.928988 0.492 41.7401 6.8675 2 2.82058 0.170225 0.725868 A F 7.03e+20 4.20491e-14 1 dx
Report 2 X101931.41-140733.6 chandra ccd7 1036.75 861.5 3.92941 2 0.00383383 0.00195135 9.18169 0.999999 0.735713 0.492 16.0531 6.06214 F F 7.03e+20 0 1 d
Report 3 X101940.35-140735.2 chandra ccd7 772.5 858.5 2.96102 1.73205 0.002889 0.00168992 6.9189 0.999959 0.673699 0.492 153.435 4.66691 F F 7.02e+20 0 1 d
Report 5 X101951.71-141206.3 chandra ccd7 436.5 307.5 2.9584 1.73205 0.00288644 0.00168992 6.91276 0.999959 0.521845 0.492 90 0.638469 F F 6.95e+20 0 1 d
Report 4 X101952.53-140849.5 chandra ccd7 412.5 707.5 0.99108 1 0.000966972 0.000975676 2.31581 0.985142 0.492 0.492 90 2.8777 F F 6.99e+20 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