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 1 X175316.45-283812.9 chandra ccd3 562.693 262.242 29.9779 5.56778 0.0138786 0.00257767 65.9209 1 1.85275 1.13104 54.2211 7.43223 A F 7.56e+21 2.11651e-13 1 dx
Report srcpi bgdpi arf 2 X175321.28-283159.3 chandra ccd3 434.413 1022.18 18.4445 4.29471 0.00853917 0.0019883 40.5592 1 0.845143 0.432801 89.9692 3.30234 F F 7.72e+21 1.23038e-13 1 dsx
Report srcpi bgdpi arf 3 X175323.79-283325.0 chandra ccd3 366.625 847.5 7.95444 2.82843 0.00368261 0.00130945 17.4917 1 0.492 0.492 180 3.00532 F F 7.63e+21 5.52917e-14 1 dx
Report 1 X175342.31-283531.2 chandra ccd1 914.75 767 3.98127 2 0.00184318 0.000925924 8.53453 0.999997 0.548732 0.492 30.9107 3.58217 F F 7.31e+21 0 1 d
Report 3 X175339.81-282931.7 chandra ccd2 141.5 291.75 3.97966 2 0.00184243 0.000925924 8.6591 0.999997 0.588072 0.492 28.3626 2.7734 F F 7.49e+21 0 1 d
Report 1 X175346.41-283016.9 chandra ccd0 987.75 405.75 3.96173 2 0.00183677 0.000927255 8.79215 0.999998 0.5535 0.492 168.69 2.93084 F F 7.39e+21 0 1 d
Report srcpi bgdpi arf 2 X175324.23-282709.6 chandra ccd2 559 580.5 3.95696 2 0.00183192 0.000925925 8.60971 0.999997 0.492 0.492 90 5.68533 F F 7.91e+21 2.87357e-14 1 dx
Report srcpi bgdpi arf 2 X175406.37-282743.2 chandra ccd0 452.5 717.75 3.83663 2.00001 0.00177877 0.000927257 8.51451 0.999998 0.699805 0.492 133.212 7.98056 F F 7.32e+21 2.7245e-14 1 dx
Report 3 X175348.01-283012.6 chandra ccd0 944.75 414.5 3.97576 2 0.00184327 0.000927255 8.82327 0.999998 0.492 0.492 145.278 3.24988 F F 7.38e+21 0 1 d
Report 3 X175338.75-283646.7 chandra ccd1 1009.83 613.5 2.95381 1.73205 0.0013675 0.000801875 6.33199 0.999921 0.529672 0.492 79.722 4.61987 F F 7.31e+21 0 1 d
Report 2 X175339.26-283543.8 chandra ccd1 996.167 741.5 2.94621 1.73205 0.00136398 0.000801875 6.31571 0.999921 0.510281 0.492 28.155 3.59835 F F 7.33e+21 0 1 d
Report srcpi bgdpi arf 1 X175325.14-283125.7 chandra ccd2 534.5 60 1.98223 1.41421 0.000917699 0.000654728 4.31302 0.998658 0.492 0.492 90 2.56375 F F 7.69e+21 1.63483e-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