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 4 X173629.96-283711.1 chandra ccd3 249.333 223.917 11.4787 3.46411 0.00532942 0.00160834 22.7904 1 1.25317 0.866558 55.2316 6.79574 F F 5.87e+21 7.75903e-14 1 dx
Report srcpi bgdpi arf 1 X173624.95-282502.6 chandra ccd2 367.944 674.611 8.8126 3 0.00408568 0.00139086 18.3778 1 0.567254 0.492 51.7479 5.91036 F F 5.41e+21 5.55359e-14 1 dx
Report srcpi bgdpi arf 1 X173617.57-283417.6 chandra ccd3 581.25 576.5 7.86303 2.82843 0.00365069 0.0013132 15.6116 1 0.727947 0.492 114.12 5.44943 F F 5.61e+21 5.12629e-14 1 dx
Report srcpi bgdpi arf 2 X173714.30-283403.6 chandra ccd1 118.25 580.375 6.96827 2.82845 0.00323062 0.00131132 14.0372 1 2.22563 1.41321 77.4828 9.26671 A F 6.27e+21 5.02352e-14 1 dx
Report srcpi bgdpi arf 2 X173605.36-283232.2 chandra ccd3 908.5 790.333 5.845 2.44949 0.00271375 0.00113727 11.6049 1 0.630188 0.550073 143.13 6.89944 F F 5.45e+21 4.02274e-14 1 dx
Report 3 X173615.91-283310.0 chandra ccd3 625.7 713.9 4.93026 2.23607 0.00228905 0.00103818 9.78877 1 0.762288 0.492 158.368 5.03796 A F 5.55e+21 0 1 d
Report srcpi bgdpi arf 1 X173711.60-283027.0 chandra ccd1 189.9 1020.7 4.85568 2.23607 0.00225118 0.00103668 9.78151 1 1.11132 0.492 3.33994 7.96311 A F 6.11e+21 3.33243e-14 1 dx
Report 2 X173631.23-282800.0 chandra ccd2 199.5 314 3.96553 2 0.00183849 0.000927238 8.26973 0.999996 0.492 0.492 106.845 2.65237 F F 5.51e+21 0 1 d
Report 6 X173632.50-282838.8 chandra ccd2 165.5 235.25 3.94889 2 0.00183078 0.000927238 8.23502 0.999996 0.492 0.492 18.652 1.95067 F F 5.55e+21 0 1 d
Report srcpi bgdpi arf 1 X173647.39-282449.0 chandra ccd0 799.25 666.25 3.896 2 0.00180626 0.000927239 8.41144 0.999997 1.03261 0.492 54.3629 6.26309 A F 5.61e+21 2.61609e-14 1 dx
Report 2 X173647.71-282223.4 chandra ccd0 790.5 962.1 4.87685 2.23607 0.002261 0.00103668 10.5291 1 0.972665 0.669486 129.96 8.54625 F F 5.55e+21 0 1 d
Report 3 X173659.66-282556.4 chandra ccd0 470.5 529 3.88733 2 0.00180224 0.000927239 8.39272 0.999997 0.492 0.492 31.7175 7.01796 F F 5.81e+21 0 1 d
Report 4 X173613.59-282621.9 chandra ccd2 672.5 513.167 2.93904 1.73205 0.00136259 0.000803012 6.12907 0.999903 1.18145 0.492 52.1907 6.31799 A F 5.38e+21 0 1 d
Report 3 X173617.68-282507.4 chandra ccd2 562.833 664.833 2.92144 1.73205 0.00135443 0.000803013 6.09237 0.999903 0.563657 0.492 45 6.62794 F F 5.38e+21 0 1 d
Report srcpi bgdpi arf 5 X173608.44-283022.3 chandra ccd2 810 24.5 1.9617 1.41422 0.000909483 0.000655657 4.09094 0.998293 0.492 0.492 116.565 5.9134 F F 5.41e+21 1.3062e-14 1 dx
Report 3 X173654.12-283431.8 chandra ccd1 658.5 523.5 1.95378 1.41422 0.00090581 0.000655657 3.9358 0.997924 0.521845 0.492 45 5.76958 F F 6.05e+21 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