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 X170544.73-410045.9 chandra ccd7 1016.68 896.211 20.5982 4.53852 0.00855586 0.00188516 28.2399 1 1.71064 0.844413 328.464 4.96566 F F 1.46e+22 1.24875e-13 1 dsx
Report srcpi bgdpi arf 3 X170545.61-410417.5 chandra ccd7 996.337 466.235 11.7498 3.4278 0.00488048 0.00142379 16.1089 1 0.794869 0.290706 343.55 2.17617 F F 1.45e+22 6.64618e-14 1 dsx
Report srcpi bgdpi arf 2 X170545.50-410402.7 chandra ccd7 998.389 495.722 8.87938 3 0.00368818 0.00124609 12.1735 1 0.492 0.492 73.155 2.31363 F F 1.45e+22 5.17017e-14 1 dx
Report srcpi bgdpi arf 1 X170509.94-411802.3 chandra ccd5 1056.08 733.083 8.10536 3.46419 0.00336668 0.0014389 9.61837 1 4.15263 2.8144 4.40445 15.4379 F F 1.45e+22 7.18267e-14 1 dx
Report srcpi bgdpi arf 1 X170532.34-410717.9 chandra ccd6 902.5 1045.83 2.97466 1.73205 0.00123557 0.000719433 6.44712 0.999928 0.492 0.492 151.845 4.89527 F F 1.45e+22 2.07017e-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