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 4 X165111.63-440238.8 chandra ccd7 149.577 625.217 149.366 12.3748 0.0810901 0.00671821 76.9339 1 0.511775 0.511775 0 1.05428 F F 1.59e+22 1.09025e-12 1 dsxf
Report srcpi bgdpi arf 2 X165037.83-440129.5 chandra ccd7 890 765.125 7.75768 2.82843 0.0042116 0.00153554 3.99575 0.999448 0.803362 0.492 57.0562 5.61507 A F 1.56e+22 6.28977e-14 1 dx
Report 1 X165047.55-440138.9 chandra ccd7 677 746.25 3.95254 2 0.00214582 0.00108579 2.03584 0.961429 0.492 0.492 136.431 3.9399 F F 1.57e+22 0 1 d
Report 3 X165039.48-435911.2 chandra ccd7 854.25 1046.25 3.76912 2.00001 0.00204624 0.00108579 1.94136 0.961429 0.492 0.492 71.565 6.51228 F F 1.55e+22 0 1 d
Report 1 X165128.02-440133.8 chandra ccd6 789.833 900.5 2.98193 1.73205 0.00161887 0.000940322 7.15929 0.999967 0.492 0.492 180 4.13275 F F 1.6e+22 0 1 d
Report 2 X165158.49-440621.2 chandra ccd6 123.3 315.1 4.86111 2.23607 0.00263907 0.00121395 11.671 1 0.492 0.492 54.2175 9.66969 F F 1.64e+22 0 1 d

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