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 arf 3 X082223.88-425760.0 chandra ccd6 316.244 428.748 271.338 55.6521 0.0238942 0.00490076 6.89461 1 4.12543 4.12543 0 8.05819 F F 7.11e+21 3.22889e-13 1 dsx
Report arf 7 X082232.57-425801.8 chandra ccd6 122.049 424.229 105.201 26.2694 0.00926403 0.00231329 2.67312 0.996089 1.66638 1.46008 47.5399 9.50881 F F 7.14e+21 1.3014e-13 1 dx
Report arf 14 X082220.68-425723.1 chandra ccd6 387.182 503.257 142.633 27.0755 0.0125603 0.00238428 3.62425 0.999825 2.51227 2.3172 139.339 7.83717 F F 7.11e+21 1.70306e-13 1 dx
Report arf 15 X082157.40-430016.8 chandra ccd6 907.191 151.496 8047.65 91.2112 0.708681 0.00803212 204.488 1 0.661818 0.661818 0 2.70889 F F 6.99e+21 8.44517e-12 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