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 2 X170144.27-405130.0 chandra ccd7 496.616 276.414 153.972 13.8078 0.151352 0.0135728 35.9516 1 1.94245 1.94245 0 0.284936 T F 1.28e+22 3.0094e-12 1 dsxf
Report srcpi bgdpi arf 1 X170156.80-404938.2 chandra ccd7 207.526 503.37 32.9556 5.7407 0.0323947 0.00564299 7.69494 1 0.798794 0.414312 296.825 3.23505 F F 1.28e+22 4.31691e-13 1 dsx
Report 1 X170152.15-405929.5 chandra ccd6 413.833 321.167 2.93541 1.73205 0.00288535 0.00170251 7.43202 0.999978 0.492 0.492 45 7.87727 F F 1.33e+22 0 1 d
Report srcpi bgdpi arf 1 X170107.42-405740.8 chandra ccd2 70.5 499.5 1 1 0.000982943 0.000982943 3.16679 0.995347 0.492 0.492 90 9.08315 F F 1.28e+22 1.83147e-14 1 dx
Report srcpi bgdpi arf 2 X170055.01-405320.7 chandra ccd2 357.5 1027.5 6.83634 2.64575 0.00671974 0.00260063 21.6493 1 1.39213 1.0471 16.845 9.38067 F F 1.24e+22 1.20939e-13 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