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 X154309.87-564037.3 chandra ccd2 913.125 700.25 7.36959 2.82844 0.00635568 0.0024393 21.8269 1 2.22015 1.05804 41.8741 8.33811 A T 1.41e+22 1.26651e-13 1 dx
Report 2 X154307.55-564139.3 chandra ccd2 951.643 574.071 6.96122 2.64575 0.00600349 0.00228175 20.6174 1 0.504301 0.492 142.876 8.0641 F F 1.41e+22 0 1 d
Report 1 X154351.92-564645.7 chandra ccd3 334.5 955.7 4.99286 2.23607 0.00430594 0.00192843 15.1093 1 0.492 0.492 90 1.66939 F T 1.34e+22 0 1 d
Report srcpi bgdpi arf 1 X154404.06-564024.3 chandra ccd0 1024.5 541 3.93441 2 0.00339311 0.00172484 12.4855 1 0.767978 0.492 121.717 5.08288 A T 1.37e+22 6.19028e-14 1 dx

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