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 X124053.60-364512.9 chandra ccd7 254.996 482.539 11.6674 4.77457 0.00133927 0.000548059 2.82136 0.994613 0.533728 0.239447 118.92 0.402721 F F 5.85e+20 9.2869e-15 1 dsx
Report srcpi bgdpi arf rmf 2 X124052.85-364521.2 chandra ccd7 273.137 465.55 276.535 17.7861 0.0317427 0.00204162 66.8705 1 0.502691 0.502691 0 0.583661 F F 5.86e+20 1.34171e-13 1 dsxf
Report srcpi bgdpi arf 3 X124038.77-364719.8 chandra ccd7 616.357 223.786 8.14169 3.00002 0.000934561 0.000344364 1.96879 0.973156 0.513331 0.497785 67.5 4.01099 F F 5.86e+20 6.82694e-15 1 dx
Report srcpi bgdpi arf 4 X124049.55-364557.3 chandra ccd7 353.677 392.099 8.87332 3.03912 0.00101854 0.000348852 2.14571 0.973156 0.406072 0.406072 0 1.4573 F F 5.86e+20 7.14229e-15 1 dsx

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