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 1 X171659.55-624914.0 chandra ccd7 238.865 151.161 3119.11 57.4557 0.318878 0.0058739 487.327 1 0.465402 0.465402 0 0.282764 F F 7.79e+20 1.10916e-11 1 dsxf
Report srcpi bgdpi arf rmf 3 X171648.23-624923.9 chandra ccd7 396.53 130.921 155.982 12.783 0.0159466 0.00130686 24.3705 1 0.427411 0.427411 0 1.57106 F F 7.81e+20 1.20417e-13 1 dsx
Report srcpi bgdpi arf rmf 2 X171705.43-624910.7 chandra ccd7 157.028 157.895 129.844 11.6236 0.0132744 0.00118832 20.2867 1 0.400928 0.400928 0 0.429713 F F 7.77e+20 1.00592e-13 1 dsx
Report srcpi bgdpi arf 6 X171706.10-624923.7 chandra ccd7 147.637 131.372 26.0307 5.86125 0.00266122 0.000599217 4.06701 0.999883 0.31862 0.31862 0 0.580056 F F 7.77e+20 2.01581e-14 1 dsx
Report srcpi bgdpi arf 4 X171652.74-624901.0 chandra ccd7 333.795 177.557 23.392 5.01663 0.00239145 0.000512868 3.65475 0.999679 0.557059 0.557059 0 1.03151 F F 7.8e+20 1.80072e-14 1 dsx
Report srcpi bgdpi arf 1 X171802.65-624913.4 chandra ccd6 394.667 234.167 10.1862 3.46413 0.00104137 0.000354149 9.2992 1 1.45279 0.97816 111.238 6.9577 F F 7.66e+20 1.2636e-14 1 dx
Report srcpi bgdpi arf 2 X171809.57-624954.6 chandra ccd6 298.667 150 8.52002 3.46416 0.000871029 0.000354152 7.77812 0.999999 3.02145 1.55864 69.331 7.7877 A F 7.64e+20 1.00208e-14 1 dx
Report srcpi bgdpi arf 3 X171728.91-624859.8 chandra ccd6 864.5 263.25 7.72552 2.82843 0.000789805 0.00028916 7.05281 0.999995 0.878894 0.492 33.7919 3.10533 A F 7.73e+20 8.21686e-15 1 dx
Report srcpi bgdpi arf 4 X171722.04-624901.9 chandra ccd6 960.167 259 5.83614 2.44949 0.000596646 0.000250419 5.32794 0.999963 0.492 0.492 111.355 2.32016 F F 7.74e+20 6.1116e-15 1 dx
Report srcpi bgdpi arf 5 X171746.26-624925.7 chandra ccd6 623 210 3.45101 2.00002 0.000352808 0.000204468 3.15051 0.992258 0.492 0.492 90 5.0951 F T 7.7e+20 3.90746e-15 1 dx
Report srcpi bgdpi arf 6 X171725.91-625015.2 chandra ccd6 906.5 110 5.86061 2.44949 0.000599148 0.000250419 5.35028 0.999963 0.492 0.492 90 2.99174 F F 7.74e+20 6.19935e-15 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