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 X231032.18-435255.0 chandra ccd7 384.912 69.3309 30.5272 7.36687 0.00114129 0.000275417 2.60249 0.99474 1.37948 1.37948 0 6.19133 F F 1.12e+20 8.16271e-15 1 dsx
Report srcpi bgdpi arf rmf 3 X231041.76-434734.2 chandra ccd7 174.483 721.434 12865.1 115.65 0.480974 0.00432368 1096.77 1 0.415522 0.394115 132.88 0.585476 F F 1.11e+20 2.94978e-12 1 dsxf
Report srcpi bgdpi arf 4 X231043.50-434741.4 chandra ccd7 136.119 706.74 33.7868 6.2621 0.00126315 0.000234114 2.88038 0.997416 2.96002 0.370003 160.834 0.626688 A F 1.11e+20 8.10735e-15 1 dscx
Report srcpi bgdpi arf 6 X231043.16-434740.0 chandra ccd7 143.686 709.717 26.7195 6.17489 0.000998935 0.000230854 2.27788 0.987404 1.48001 1.48001 0 0.597356 T F 1.11e+20 6.41732e-15 1 dscx

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