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 X142828.42-022645.0 chandra ccd0 380.912 946.853 15.7979 4.12313 0.00647875 0.0016909 40.2594 1 2.09135 1.74443 167.362 9.56487 F F 3.94e+20 9.38161e-14 1 dx
Report srcpi bgdpi arf 2 X142808.89-023124.9 chandra ccd0 976.189 378.357 18.1762 4.26336 0.00745415 0.00174842 46.3203 1 0.925967 0.542597 0.114858 3.76725 F F 4.04e+20 8.84113e-14 1 dsx
Report srcpi bgdpi arf 1 X142755.60-023029.1 chandra ccd2 486.5 39.3335 5.93047 2.44949 0.0024321 0.00100454 14.6899 1 0.501669 0.492 160.032 0.596352 F F 4.05e+20 2.74231e-14 1 dx
Report 1 X142803.61-023652.9 chandra ccd1 689.5 675.167 2.93715 1.73205 0.00120453 0.000710318 7.48928 0.999979 0.54799 0.492 56.9812 6.43829 F F 4.13e+20 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