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 X123922.91-003559.1 chandra ccd7 534.167 214.833 2.75213 1.73206 0.00128856 0.000810962 4.18089 0.998959 0.492 0.492 106.845 6.05297 F F 1.83e+20 0 1 d
Report 2 X123902.34-003204.6 chandra ccd7 1161.25 691.5 3.90888 2 0.00183016 0.000936415 5.93817 0.999911 0.602813 0.492 32.6882 5.56496 F F 1.83e+20 0 1 d
Report 3 X123909.58-003138.2 chandra ccd7 940.5 745.1 4.87274 2.23607 0.00228145 0.00104694 7.40243 0.999994 0.645643 0.492 83.8676 3.73665 F F 1.83e+20 0 1 d
Report 4 X123907.81-003101.8 chandra ccd7 994.5 819 1.93996 1.41422 0.000908304 0.000662146 2.94709 0.990167 0.492 0.492 153.435 3.92485 F F 1.84e+20 0 1 d
Report 5 X123904.79-003221.2 chandra ccd7 1086.75 657.75 3.93389 2 0.00184188 0.000936414 5.97618 0.999911 0.492 0.492 90 5.1314 F F 1.83e+20 0 1 d
Report 6 X123920.05-003147.5 chandra ccd7 621.908 726.71 14.3168 3.78375 0.00670338 0.00177162 21.7494 1 0.702729 0.290392 103.237 1.99045 F F 1.84e+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