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 X040749.11-121132.4 chandra ccd7 369.302 727.662 53.4953 7.50838 0.00617617 0.000866863 4.67465 0.999995 1.44026 1.44026 0 0.277508 T F 3.48e+20 0 1 ds
Report 2 X040748.60-121118.2 chandra ccd7 384.727 756.518 30.8894 6.8683 0.00356627 0.000792965 2.69925 0.995175 0.444502 0.444502 0 0.0766856 F F 3.48e+20 0 1 ds
Report 3 X040747.21-121145.1 chandra ccd7 426.132 701.889 30.8445 5.87594 0.00356108 0.000678392 2.69533 0.995175 1.5 0.547787 205.579 0.47486 A F 3.48e+20 0 1 ds
Report 5 X040748.42-121136.7 chandra ccd7 389.847 719.02 11093.2 108.223 1.28074 0.0124947 969.372 1 0.417527 0.417527 0 0.267226 F T 3.48e+20 0 1 ds
Report 7 X040749.81-121127.1 chandra ccd7 348.511 738.501 27.8764 6.38011 0.00321841 0.000736601 2.43596 0.990438 1.25895 1.25895 0 0.399757 T F 3.47e+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