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 X221023.01-300113.5 chandra ccd7 1084.15 1009.82 12.9335 3.59632 0.00852291 0.0023699 24.3409 1 0.572439 0.572439 0 2.96751 7 4 -0.272727 0.42065 F F 1.28e+20 8.77108e-14 1 dsx
Report 1 X221038.71-295931.6 chandra ccd6 342 219.667 5.98921 2.44949 0.00394674 0.00161415 17.3361 1 0.492 0.492 108.435 2.25382 F F 1.26e+20 0 1 d
Report srcpi bgdpi arf 4 X221046.01-300158.1 chandra ccd7 476.5 918.75 3.83061 3.17945 0.00252428 0.00209518 9.30741 0.999999 0.492 0.492 28.9973 2.06806 3 -0.0846933 -1 1.41421 F F 1.25e+20 1.90059e-14 1 dx
Report 3 X221056.49-300443.6 chandra ccd7 200.167 582.167 2.95177 1.73205 0.00194514 0.00114138 5.55523 0.999789 0.563657 0.492 45 5.25944 F F 1.23e+20 0 1 d
Report 2 X221043.12-300814.9 chandra ccd7 552.833 152.833 2.84917 1.73206 0.00187753 0.00114138 5.36215 0.999789 0.492 0.492 19.9028 6.67494 F F 1.24e+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