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 X031822.28-663603.6 chandra ccd7 360.307 312.066 1098.75 33.8552 0.236133 0.00727585 273.559 1 0.431241 0.431241 0 0.580844 F F 4.16e+20 0 1 ds
Report 2 X031818.49-663003.1 chandra ccd7 406.246 1044.83 119.857 10.9479 0.0257586 0.00235283 29.8412 1 2.60042 2.60042 0 6.55664 F F 4.13e+20 0 1 ds
Report 1 X031818.91-663230.5 chandra ccd7 401.112 745.296 17.696 4.32074 0.00380305 0.000928572 4.40583 0.99993 1.02061 1.02061 0 4.10422 F F 4.14e+20 0 1 ds
Report 1 X031822.45-663947.3 chandra ccd6 189.75 876 3.96233 2 0.000851545 0.00042982 7.19171 0.999983 0.670703 0.492 98.1569 3.18887 F F 4.16e+20 0 1 d
Report 2 X031802.28-663908.8 chandra ccd6 433.5 954 1.95284 1.41422 0.000419685 0.000303929 3.54445 0.996281 0.492 0.492 26.5651 3.10526 F F 4.13e+20 0 1 d
Report 3 X031756.77-664051.2 chandra ccd6 499.75 745.75 3.93005 2 0.000844608 0.000429821 7.13312 0.999983 0.5535 0.492 30.9638 4.84492 F F 4.12e+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