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 rmf 2 X200913.10-853844.3 chandra ccd7 915.832 511.342 308.816 17.9986 0.15387 0.00896793 79.3801 1 0.411643 0.411643 0 0.323198 F F 8.93e+20 1.44455e-12 1 dsxf
Report srcpi bgdpi arf 1 X200736.90-852941.3 chandra ccd3 264.5 507.75 3.72998 2.00001 0.00185846 0.000996502 9.7413 0.999983 1.51226 0.492 101.462 9.54004 A F 8.92e+20 2.53432e-14 1 dx
Report srcpi bgdpi arf 2 X200716.64-852613.2 chandra ccd3 316.5 930.3 4.81021 2.23607 0.00239668 0.00111412 12.5625 1 2.44759 0.492 85.7633 13.0247 A F 8.92e+20 3.50082e-14 1 dx
Report srcpi bgdpi arf 1 X200434.50-854218.0 chandra ccd6 824.5 815.167 2.84299 1.73206 0.00141652 0.000862995 7.03949 0.999974 1.0936 0.492 43.5322 6.12392 A F 8.83e+20 1.67389e-14 1 dx
Report srcpi bgdpi arf 2 X200320.57-854321.2 chandra ccd6 990 683 1.96988 1.41421 0.000981488 0.000704631 4.87759 0.99936 0.492 0.492 45 7.8531 F F 8.8e+20 1.15065e-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