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 X060759.70-083450.1 chandra ccd7 240.545 257.543 6930.63 85 0.261821 0.00321107 723.926 1 0.410186 0.410186 0 0.289734 F F 1.83e+21 2.38419e-12 1 dscxf
Report srcpi bgdpi arf rmf 2 X060759.88-083450.2 chandra ccd7 235.314 257.342 554.125 24.7037 0.0209334 0.000933241 57.8801 1 1.1953 1.1953 0 0.256555 T F 1.83e+21 1.67643e-13 1 dscx
Report srcpi bgdpi arf 3 X060740.44-083556.0 chandra ccd7 821.078 123.521 54.7276 7.47379 0.00206746 0.00028234 5.71647 1 1.36605 1.36605 0 5.13027 F F 1.82e+21 1.74258e-14 1 dsx
Report srcpi bgdpi arf 5 X060751.89-083523.0 chandra ccd7 476.058 190.522 25.0494 6.32688 0.000946302 0.000239013 2.61649 0.993897 0.677114 0.677114 0 2.26321 F F 1.83e+21 7.70001e-15 1 dsx
Report srcpi bgdpi arf rmf 9 X060743.18-083602.5 chandra ccd7 738.099 109.744 186.304 14.0357 0.00703806 0.000530232 19.46 1 0.862169 0.551404 112.788 4.51078 A F 1.82e+21 5.88451e-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