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 X205741.07-440325.4 chandra ccd7 55.5677 763.661 11.5224 4.72023 0.000504612 0.000206718 6.04314 0.999999 0.695986 0.695986 0 4.5206 F F 3.05e+20 4.11443e-15 1 dsx
Report srcpi bgdpi arf 2 X205739.77-440751.3 chandra ccd7 84.0752 223.206 14.9634 3.91641 0.000655305 0.000171515 7.84784 1 0.46612 0.46612 0 0.124122 F F 3.03e+20 4.66211e-15 1 dsx
Report srcpi bgdpi arf 3 X205739.29-440550.5 chandra ccd7 94.4182 468.846 11.839 3.98858 0.000518476 0.000174675 6.20919 0.999999 0.349857 0.349857 0 2.08443 F F 3.04e+20 3.72681e-15 1 dsx
Report srcpi bgdpi arf 4 X205737.21-440201.1 chandra ccd7 139.5 934.5 6.90287 3.00006 0.000302302 0.000131383 3.62034 0.998628 0.492 0.492 90 5.91886 F F 3.06e+20 4.63698e-15 1 dx
Report srcpi bgdpi arf 5 X205738.11-440853.3 chandra ccd7 120.244 97.2147 12.723 3.56693 0.000557189 0.00015621 6.67282 1 0.319073 0.319073 0 0.9811 F F 3.02e+20 4.00893e-15 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