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 3 X113151.58-123158.5 chandra ccd7 223.452 103.495 1167.24 34.8847 0.262884 0.00785667 285.528 1 0.788915 0.788915 0 0.0989694 T F 3.42e+20 0 1 dsc
Report 1 X113151.50-123158.8 chandra ccd7 225.61 102.845 908.12 30.135 0.204525 0.00678695 222.142 1 1.45329 1.02734 359.166 0.140721 T F 3.42e+20 0 1 dscb
Report 2 X113149.05-123138.6 chandra ccd7 298.557 143.854 10.0739 3.24194 0.00226881 0.000730139 2.46426 0.987514 0.388403 0.388403 0 0.792385 F F 3.41e+20 0 1 ds
Report 2 X113204.93-124335.4 chandra ccd2 99.8999 519.4 6.56315 3.16235 0.00147813 0.000712213 11.0802 1 2.82194 1.94716 127.964 11.9752 F F 3.51e+20 0 1 d
Report 3 X113205.07-124350.8 chandra ccd2 95.7593 488.093 19.943 5.19624 0.00449149 0.00117028 33.6686 1 4.46379 3.41798 29.7279 12.2317 F F 3.51e+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