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 2 X175359.84-292907.4 chandra ccd2 260.303 135.269 64.8081 8.05035 0.0333311 0.00414033 46.6623 1 5.69184 3.76957 57.1543 9.70279 17.6424 44.9253 0.436053 0.159088 F F 5.43e+21 5.45101e-13 1 dsx
Report srcpi bgdpi arf 1 X175253.15-292209.3 chandra ccd0 1001.63 908.546 43.9081 6.88947 0.0225465 0.0035377 23.2822 1 4.38134 3.14323 31.955 9.10376 13.3925 32.271 0.413426 0.187875 F F 6.5e+21 3.58013e-13 1 dsx
Report srcpi bgdpi arf 1 X175356.35-292828.5 chandra ccd2 353.063 214.345 10.4674 3.78488 0.00538342 0.00194658 7.5366 1 1.45657 1.45657 0 8.72477 5.83066 4.66132 -0.111451 0.428112 F F 5.5e+21 8.34316e-14 1 dsx
Report 6 X175348.69-292229.3 chandra ccd2 555.375 944.125 7.96313 2.82843 0.00409537 0.00145464 5.73351 0.999965 0.618236 0.492 99.7791 3.35722 F F 5.77e+21 0 1 d
Report 3 X175344.28-291959.7 chandra ccd3 763.5 248.1 4.93798 2.23607 0.00253547 0.00114814 10.9031 1 0.612166 0.492 62.8769 2.41492 F F 5.89e+21 0 1 d
Report srcpi bgdpi arf 2 X175324.94-292301.0 chandra ccd0 156.3 803.7 4.91531 3.39792 0.00252398 0.00174481 16.8899 1 0.492 0.492 149.527 2.80295 4 0.915307 -0.627569 0.828535 F F 6.05e+21 3.31753e-14 1 dx
Report srcpi bgdpi arf 3 X175326.13-292255.9 chandra ccd0 124.9 814.1 4.91531 3.39792 0.00252398 0.00174481 16.8899 1 0.492 0.492 56.3099 2.5562 -0.0846933 5 1 0.975663 F F 6.04e+21 3.75706e-14 1 dx
Report 3 X175315.90-292005.9 chandra ccd1 488.75 125.5 3.98135 2 0.00204436 0.00102697 8.6036 0.999997 0.492 0.492 180 4.19949 F F 6.24e+21 0 1 d
Report srcpi bgdpi arf 4 X175340.25-292303.1 chandra ccd2 779.75 875.5 3.83061 3.17945 0.00197005 0.00163516 9.30741 0.999999 0.492 0.492 90 2.26755 2 1.83061 -0.0442192 0.845617 F F 5.86e+21 2.95495e-14 1 dx
Report 2 X175340.42-291644.7 chandra ccd3 866 644.5 3.95505 2 0.00203077 0.00102692 8.73278 0.999997 0.492 0.492 16.845 4.58938 F F 6.02e+21 0 1 d
Report 2 X175317.26-291832.9 chandra ccd1 452.75 314.5 3.95009 2 0.00202831 0.00102697 8.53606 0.999997 0.636736 0.492 32.2961 4.58156 F F 6.26e+21 0 1 d
Report 5 X175310.07-292120.5 chandra ccd0 551.5 1007.75 3.93968 2 0.002023 0.00102699 2.08901 0.971015 0.514845 0.492 149.221 5.33751 F F 6.27e+21 0 1 d
Report srcpi bgdpi arf 6 X175257.44-292344.7 chandra ccd0 886.833 714.167 5.59987 3.59808 0.0028755 0.00184759 8.8527 1 1.81246 0.951692 70.727 8.49106 4.68879 0.911082 -0.674606 0.785335 A F 6.4e+21 4.45911e-14 1 dx
Report 1 X175321.11-291909.0 chandra ccd1 350.5 241.167 2.96094 1.73205 0.00152039 0.00088938 6.39851 0.999926 0.492 0.492 151.845 3.54998 F F 6.2e+21 0 1 d
Report 1 X175334.99-291759.8 chandra ccd3 1010.5 491.833 2.95491 1.73205 0.00151724 0.000889343 6.52448 0.999937 0.602575 0.492 2.48675e-08 3.15704 F F 6.05e+21 0 1 d
Report 4 X175359.95-292007.0 chandra ccd3 347 233 1.96966 1.41421 0.00101134 0.000726146 4.34902 0.998766 0.492 0.492 45 5.63061 F F 5.68e+21 0 1 d
Report srcpi bgdpi arf 9 X175322.13-292400.7 chandra ccd0 231.071 682.357 6.93244 3.78388 0.00355977 0.001943 26.672 1 0.616646 0.492 157.5 3.93684 6.93244 0 -1 0.780996 F F 6.06e+21 4.79252e-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