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 X120800.86-273112.4 chandra ccd3 940.351 762.677 16.6095 4.07548 0.008536 0.00209448 42.8168 1 0.886857 0.886857 0 4.43695 F F 7.19e+20 1.00287e-13 1 dsx
Report 1 X120731.21-272628.0 chandra ccd1 744 1016 3.91167 2 0.00201028 0.00102784 10.6336 1 0.492 0.492 45 9.62655 F F 7.27e+20 0 1 d
Report 3 X120752.52-273413.1 chandra ccd3 1165.5 394.833 2.97724 1.73205 0.00153005 0.000890131 7.67486 0.999981 0.492 0.492 90 0.900495 F F 7.21e+20 0 1 d
Report 1 X120805.07-273634.0 chandra ccd2 495.5 1076.5 1.98977 1.41421 0.00102258 0.000726789 5.03222 0.999433 0.492 0.492 90 3.48588 F F 7.19e+20 0 1 d
Report srcpi bgdpi arf 2 X120814.21-273642.3 chandra ccd3 579.5 91.5 0.992915 1 0.000510276 0.000513917 2.55958 0.989752 0.492 0.492 90 5.4224 F F 7.18e+20 1.02665e-14 1 dx

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