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 2 X042035.41-204646.4 chandra ccd7 811.735 894.678 77.5067 9.23246 0.0186978 0.00222724 44.5398 1 0.365029 0.365029 0 1.52554 F T 2.35e+20 0 1 ds
Report 1 X042034.65-204626.6 chandra ccd7 833.603 934.962 46.36 6.80882 0.0111839 0.00164256 26.6411 1 0.384311 0.384311 0 1.61035 F F 2.35e+20 0 1 ds
Report 5 X042032.09-204759.4 chandra ccd7 906.556 746.402 47.2288 7.21408 0.0113935 0.00174033 27.1404 1 0.411575 0.411575 0 0.586924 F F 2.34e+20 0 1 ds
Report 4 X042052.36-205202.9 chandra ccd7 328.5 250.773 18.6711 4.69047 0.00424537 0.0010665 10.7295 1 2.05174 0.957705 152.665 6.82363 A F 2.3e+20 0 1 d
Report 3 X042030.19-204559.6 chandra ccd7 960.746 989.943 13.9831 4.02949 0.0033733 0.000972079 8.03549 1 0.392767 0.392767 0 1.65212 F F 2.36e+20 0 1 ds
Report 11 X042039.92-204940.0 chandra ccd7 683.301 541.837 11.509 3.44247 0.00277644 0.000830464 6.61373 0.999999 0.4196 0.4196 0 3.06684 F F 2.33e+20 0 1 ds
Report 7 X042046.46-204726.4 chandra ccd7 496.357 812.929 6.67199 2.64576 0.00151705 0.000601583 3.83411 0.998819 0.554038 0.492 96.6203 3.84012 F F 2.34e+20 0 1 d
Report 8 X042045.42-204648.9 chandra ccd7 526 889.167 5.81127 2.44949 0.00132134 0.000556957 3.33949 0.995963 0.492 0.492 90 3.68616 F F 2.34e+20 0 1 d
Report 10 X042048.78-204603.7 chandra ccd7 430.3 980.9 4.81254 2.23607 0.00109426 0.00050843 2.76556 0.987475 0.492 0.492 131.437 4.65343 F F 2.34e+20 0 1 d
Report 1 X042006.05-204930.4 chandra ccd6 680 109.75 3.96441 2 0.000901413 0.000454753 7.37853 0.999987 0.492 0.492 142.018 5.91025 F F 2.36e+20 0 1 d
Report 2 X042108.68-204242.0 chandra ccd3 566.5 208.5 3.75709 2.00001 0.000854273 0.000454754 7.5685 0.999994 0.492 0.492 90 10.2952 F T 2.35e+20 0 1 d
Report 1 X042106.46-204030.5 chandra ccd3 629.5 475.75 3.59224 2.00001 0.000816791 0.000454755 7.23643 0.999874 0.899424 0.492 75.7629 11.1077 A F 2.36e+20 0 1 d
Report 1 X042024.15-203850.0 chandra ccd2 894.5 255.5 0.963045 1 0.000218997 0.000227401 1.91426 0.972894 0.492 0.492 90 8.91858 F F 2.42e+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