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 rmf 10 X024104.82-081520.7 chandra ccd7 326.033 618.357 278.483 17.7976 0.118979 0.00760381 63.6614 1 0.579089 0.459604 318.912 1.75766 F T 2.83e+20 2.45431e-12 1 dsxf
Report srcpi bgdpi arf 3 X024106.03-081220.7 chandra ccd7 289.351 984.198 10.5707 3.25126 0.00451619 0.00138906 2.41647 0.987069 0.400027 0.400027 0 1.29769 F F 2.82e+20 2.61239e-14 1 dsx
Report srcpi bgdpi arf 8 X024105.80-081522.1 chandra ccd7 295.833 615.056 8.29688 3.00001 0.00354472 0.00128171 1.89667 0.966317 0.774528 0.492 62.6001 1.80626 A F 2.83e+20 2.03765e-14 1 dx
Report srcpi bgdpi arf 1 X024059.44-080639.6 chandra ccd6 366.75 634 3.9075 2 0.00166942 0.000854471 10.262 1 0.492 0.492 127.982 7.04276 F F 2.81e+20 1.66062e-14 1 dx
Report 1 X024139.05-080615.5 chandra ccd2 769.167 507.833 2.9672 1.73205 0.00126769 0.000739993 8.45784 0.999991 1.09731 0.492 164.391 11.2563 A F 2.65e+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