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 X124349.34-080248.4 chandra ccd7 587.351 863.614 161.372 13.2046 0.0432116 0.00353589 63.3184 1 0.432682 0.432682 0 0.587646 F F 2.16e+20 0 1 ds
Report 1 X124336.61-080453.6 chandra ccd7 971.779 609.26 29.2001 5.40371 0.00781909 0.00144699 11.4574 1 1.37801 0.697816 104.458 4.32175 F F 2.17e+20 0 1 ds
Report 2 X124405.91-080247.0 chandra ccd7 86.75 866.125 7.73212 2.82843 0.00207045 0.000757378 3.03389 0.997064 0.581723 0.492 91.7083 3.82004 F F 2.15e+20 0 1 d
Report 1 X124347.34-075700.8 chandra ccd6 1021.33 615.667 5.84509 2.44949 0.00156516 0.000655909 8.57453 0.999999 0.672604 0.492 19.1837 5.35551 F F 2.11e+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