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 3 X161733.20-510143.7 chandra ccd3 868.227 237.073 82.4841 16.4038 0.0212707 0.00423015 4.1052 0.999968 5.47219 5.47219 0 7.89002 T F 2.07e+22 4.30909e-13 1 dsx
Report srcpi bgdpi arf rmf 4 X161748.65-505942.3 chandra ccd3 572.134 484.238 135.744 27.9465 0.035005 0.00720673 6.75592 1 6.82484 6.82484 0 8.59184 T F 2.07e+22 2.27702e-13 1 dscxf
Report srcpi bgdpi arf 5 X161753.71-505928.4 chandra ccd3 474.577 511.961 38.0346 9.21987 0.00980813 0.00237756 1.89297 0.968601 1.65387 1.21956 68.5596 8.53927 F F 2.07e+22 2.05266e-13 1 dx
Report srcpi bgdpi arf rmf 6 X161736.24-510224.5 chandra ccd3 809.704 154.263 3571.49 64.6814 0.921001 0.0166798 177.752 1 2.03721 2.03721 0 7.06644 F F 2.07e+22 1.82784e-11 1 dsx

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