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 8 X002038.85-693730.9 chandra ccd3 49.3522 167.697 119.603 10.9363 0.0512254 0.00468397 347.106 1 1.28111 0.391211 55.8264 0.290254 A F 2.71e+20 7.28196e-13 1 dscxf
Report srcpi bgdpi arf 1 X002039.00-693729.7 chandra ccd3 47.2021 169.542 46.8113 6.85566 0.0200489 0.00293622 135.853 1 0.492 0.492 123.279 0.275407 F F 2.71e+20 2.18127e-13 1 dpcx
Report srcpi bgdpi arf 1 X002158.91-693925.6 chandra ccd0 335.2 850.8 9.60891 3.16229 0.00411542 0.00135438 27.2892 1 1.46726 1.28933 48.1877 6.93845 F F 2.69e+20 5.05487e-14 1 dx
Report 1 X002055.06-693413.8 chandra ccd2 921.389 450.722 8.93773 3 0.00382796 0.00128488 25.1865 1 0.539184 0.492 28.8622 3.53124 F F 2.69e+20 0 1 d
Report srcpi bgdpi arf 7 X001928.67-693113.0 chandra ccd3 797.611 933.278 8.28905 3.00001 0.00355013 0.00128488 24.0561 1 2.61591 1.5565 165.06 9.02164 A F 2.71e+20 4.96732e-14 1 dx
Report srcpi bgdpi arf 5 X001936.41-693521.7 chandra ccd3 712.75 428.125 7.63205 2.82844 0.00326875 0.0012114 22.1494 1 1.22297 0.798895 90.2843 6.12944 A F 2.73e+20 4.06611e-14 1 dx
Report srcpi bgdpi arf 1 X001919.83-693950.4 chandra ccd1 990.929 892.214 6.83692 2.64576 0.0029282 0.00113316 20.1675 1 1.31652 0.882496 170.308 7.49858 F F 2.75e+20 3.74862e-14 1 dx
Report srcpi bgdpi arf 2 X001918.29-694048.2 chandra ccd1 1006.67 774.667 5.72849 2.4495 0.00245347 0.0010491 16.8979 1 1.53414 0.562759 84.3242 7.96396 A F 2.76e+20 3.19247e-14 1 dx
Report 2 X002040.29-693717.8 chandra ccd3 33.5 193.7 4.96398 2.23607 0.00212603 0.000957691 14.4062 1 0.492 0.492 2.35927e-08 0.315242 F F 2.71e+20 0 1 d
Report srcpi bgdpi arf 3 X002031.53-693510.4 chandra ccd3 126.7 452.7 4.96111 2.23607 0.0021248 0.000957691 14.3979 1 0.492 0.492 154.903 2.56897 F F 2.71e+20 2.40203e-14 1 dx
Report 3 X002055.44-693754.9 chandra ccd2 917.75 1.25 3.99576 2 0.00171135 0.000856584 11.2601 1 0.492 0.492 45 1.21565 F F 2.71e+20 0 1 d
Report srcpi bgdpi arf 2 X002107.18-694253.2 chandra ccd0 884.25 430.75 3.9362 2 0.00168584 0.000856585 11.1788 1 0.54863 0.492 172.982 5.74498 F F 2.73e+20 2.00261e-14 1 dx
Report srcpi bgdpi arf 6 X001902.66-693133.6 chandra ccd3 1074.75 889.75 3.88316 2.00001 0.00166313 0.000856586 11.2695 1 2.0705 0.492 105.903 10.551 A F 2.72e+20 2.4716e-14 1 dx
Report srcpi bgdpi arf 3 X002111.69-694443.5 chandra ccd0 837 206.5 3.84707 2.00001 0.00164767 0.000856586 10.9256 0.999991 1.13151 0.769348 40.7346 7.60094 F F 2.73e+20 2.09497e-14 1 dx
Report srcpi bgdpi arf 4 X002133.71-694516.4 chandra ccd0 604.8 139.1 9.29191 3.16229 0.00397965 0.00135438 26.3889 1 3.00734 1.46804 72.4859 8.90995 A F 2.73e+20 5.23842e-14 1 dx
Report 4 X002002.07-693741.3 chandra ccd3 439.167 145.5 2.96393 1.73205 0.00126943 0.000741824 8.60176 0.999992 0.561105 0.492 115.097 3.4802 F F 2.73e+20 0 1 d
Report 2 X002136.32-693521.0 chandra ccd2 482.833 313.167 2.96226 1.73205 0.00126871 0.000741824 8.34765 0.999991 0.492 0.492 45 5.2256 F F 2.68e+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