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 1 X044203.29-011801.7 chandra ccd3 508.233 124.167 14.4984 3.87299 0.000614644 0.000164191 4.44274 0.999951 0.557363 0.492 15.4458 3.8886 F T 3.58e+20 0 1 dp
Report 2 X044154.22-011747.6 chandra ccd3 784.5 152.75 7.69702 2.82843 0.000326307 0.000119908 2.3586 0.986854 0.492 0.492 142.018 1.72221 F F 3.59e+20 0 1 d
Report 3 X044205.97-011711.0 chandra ccd3 426.5 227.167 8.72416 3.00001 0.000369851 0.000127182 2.67334 0.993299 0.492 0.492 61.845 4.70493 F F 3.58e+20 0 1 d
Report 4 X044209.52-011657.5 chandra ccd3 318.676 255.163 46.8283 7.02578 0.00198524 0.000297851 14.3496 1 1.43144 0.644806 100.341 5.6231 A F 3.58e+20 0 1 ds
Report 5 X044148.52-011648.3 chandra ccd3 958.732 273.853 40.7185 6.39413 0.00172622 0.000271073 12.4774 1 0.419352 0.419352 0 1.62829 F F 3.59e+20 0 1 ds
Report 6 X044147.67-011744.1 chandra ccd3 984.25 159.875 7.50448 2.82844 0.000318144 0.000119908 2.29959 0.986854 0.583729 0.492 65.6994 0.688657 T F 3.59e+20 0 1 d
Report 9 X044148.27-011806.7 chandra ccd3 966.352 114.525 361.616 19.7703 0.0153303 0.000838142 110.81 1 0.421118 0.367767 340.619 0.332975 F F 3.59e+20 0 1 ds

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