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 1 X222328.89-300423.2 chandra ccd3 475.38 390.371 13.1478 3.62599 0.0052027 0.00143484 15.0767 1 1.45051 1.45051 0 6.19132 F F 1.09e+20 0 1 ds
Report srcpi bgdpi arf 4 X222334.75-300350.0 chandra ccd3 320.752 458.003 11.1182 3.71955 0.00439956 0.00147186 12.7493 1 0.716528 0.716528 0 5.06098 F F 1.09e+20 5.95254e-14 1 dsx
Report srcpi bgdpi arf 3 X222313.27-295955.9 chandra ccd3 888.139 933.428 11.4279 3.42826 0.00452211 0.00135659 13.1045 1 1.36748 1.36748 0 6.93686 F F 1.08e+20 6.45586e-14 1 dsx
Report 2 X222325.48-295855.5 chandra ccd3 565.985 1056.52 9.76577 3.12502 0.0038644 0.0012366 11.1985 1 0.87448 0.278551 98.9458 4.2868 F F 1.08e+20 0 1 ds
Report srcpi bgdpi arf 2 X222402.34-300655.5 chandra ccd1 624.5 232.5 10.074 3.31664 0.0039863 0.00131241 25.5812 1 0.492 0.492 90 8.4771 F F 1.09e+20 5.96262e-14 1 dx
Report 2 X222335.97-295546.1 chandra ccd2 445.5 398 7.89571 2.82843 0.00312436 0.00111922 19.9864 1 0.728487 0.492 129.848 4.05923 F F 1.09e+20 0 1 d
Report srcpi bgdpi arf 1 X222358.06-300511.6 chandra ccd1 737.5 443.7 4.88577 2.23607 0.00193332 0.000884821 12.4066 1 1.07698 0.492 28.2378 6.51482 A F 1.09e+20 2.52888e-14 1 dx
Report srcpi bgdpi arf 1 X222335.71-295311.2 chandra ccd2 452.5 712.9 4.79151 2.23607 0.00189602 0.000884823 12.1287 0.999999 0.976707 0.492 119.219 6.45209 A F 1.09e+20 2.64595e-14 1 dx
Report 3 X222348.95-300118.3 chandra ccd1 977.75 918 3.9734 2 0.00157229 0.000791408 10.0898 0.999999 0.492 0.492 116.565 2.15999 F F 1.09e+20 0 1 d
Report 5 X222333.96-295620.6 chandra ccd2 498.5 327.833 2.95862 1.73205 0.00117074 0.000685379 7.48915 0.999978 0.54799 0.492 123.019 3.82961 F F 1.09e+20 0 1 d
Report srcpi bgdpi arf 4 X222322.79-295402.0 chandra ccd2 793.833 609.5 2.8775 1.73206 0.00113864 0.00068538 7.2838 0.999978 0.897469 0.492 61.845 7.16303 A F 1.09e+20 1.72304e-14 1 dx
Report 1 X222358.26-295424.2 chandra ccd0 891.5 740.5 1.98866 1.41421 0.00078692 0.00055961 5.39416 0.999622 0.521845 0.492 45 5.65964 F F 1.09e+20 0 1 d
Report 3 X222345.47-295153.7 chandra ccd2 194.5 870.5 0.96818 1 0.000383112 0.000395704 2.45075 0.989017 0.492 0.492 90 7.40896 F F 1.09e+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