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 7 X162209.73-500600.6 chandra ccd7 458.244 478.597 16.1475 5.05072 0.0105598 0.00330297 5.27733 0.999994 0.398721 0.398721 0 0.266803 F F 1.75e+22 1.53393e-13 1 dsx
Report srcpi bgdpi arf 5 X162155.98-495902.9 chandra ccd7 727.312 1326.94 14.7927 4.00002 0.00967355 0.00261578 4.83454 0.999984 1.72842 1.2215 25.5173 7.08737 F F 1.78e+22 1.56645e-13 1 dx
Report srcpi bgdpi arf 4 X162206.97-500458.6 chandra ccd7 511.786 604.214 6.89358 2.64575 0.004508 0.00173017 2.25296 0.984341 0.524399 0.492 52.8211 0.939764 F T 1.76e+22 6.50871e-14 1 dx
Report srcpi bgdpi arf 1 X162211.48-501101.5 chandra ccd6 1203.5 543.5 1.9792 1.41421 0.00129428 0.000924814 4.9491 0.999395 0.521845 0.492 45 5.27233 F F 1.75e+22 2.4452e-14 1 dx
Report srcpi bgdpi arf 2 X162246.14-500556.7 chandra ccd6 525.7 1162.3 4.97059 2.23607 0.00325048 0.00146226 12.4292 1 0.492 0.492 160.67 5.76214 F F 1.75e+22 5.9532e-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