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 X165005.18-495623.5 chandra ccd7 41.5 675.167 19.5287 4.58261 0.00106911 0.000250878 1.99888 0.971704 0.745936 0.492 139.872 1.31659 A F 4.35e+21 9.55508e-15 1 dpbx
Report srcpi bgdpi arf 3 X164957.18-500132.5 chandra ccd7 198.791 47.6218 76.3626 9.65452 0.00418053 0.000528543 7.81616 1 2.64596 1.81395 130.955 6.48516 F F 4.28e+21 4.18758e-14 1 dsx
Report srcpi bgdpi arf 4 X164959.69-495743.5 chandra ccd7 149.693 513.018 31.0876 5.79162 0.00170191 0.000317067 3.182 0.998825 1.5 1.5 0 2.65765 T F 4.34e+21 1.5656e-14 1 dsx
Report srcpi bgdpi arf rmf 5 X165000.94-495744.2 chandra ccd7 125.108 511.536 8865.89 95.5664 0.48537 0.00523185 907.475 1 0.595028 0.595028 0 2.63669 F T 4.34e+21 5.09161e-12 1 dsxf

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