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 X212600.67-441018.4 chandra ccd7 257.643 348.929 6.88354 2.64575 0.00179659 0.000690536 7.38726 0.999996 0.492 0.492 119.767 1.16978 F F 2.58e+20 1.28268e-14 1 dx
Report 2 X212558.55-441016.6 chandra ccd7 303.833 352.5 2.89402 1.73205 0.000755334 0.000452063 3.1058 0.988051 0.492 0.492 2.52234e-08 1.38832 F F 2.59e+20 0 1 d
Report srcpi bgdpi arf 3 X212606.82-440819.7 chandra ccd7 123.1 590.1 4.81519 2.23607 0.00125676 0.00058361 5.16756 0.999716 0.519759 0.492 18.1269 3.11737 F F 2.6e+20 9.27553e-15 1 dx
Report srcpi bgdpi arf 4 X212604.02-441119.4 chandra ccd7 184.845 225.402 60.3702 7.76983 0.0157565 0.00202791 64.788 1 0.422655 0.422655 0 0.148022 F F 2.57e+20 1.11868e-13 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