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 X024145.14+003029.4 chandra ccd7 621.089 1057.67 13.8737 3.72474 0.0219556 0.00589453 32.8702 1 2.41162 0.961571 335.026 5.70639 F F 3.04e+20 1.28546e-13 1 dsx
Report 2 X024132.37+002615.6 chandra ccd7 1010.31 541.624 7.40812 2.72179 0.0117236 0.00430733 17.5517 1 0.697148 0.697148 0 3.93662 F F 3.02e+20 0 1 ds
Report 5 X024141.02+002644.8 chandra ccd7 746.691 601 2.5956 1.61109 0.00410764 0.00254961 6.14962 0.999175 0.218001 0.218001 0 2.47184 F F 3.02e+20 0 1 ds
Report 3 X024144.07+002541.5 chandra ccd7 653.25 472 3.52717 2.00001 0.00310105 0.00175839 8.35674 0.999964 0.607607 0.492 149.089 1.16641 T F 3.01e+20 0 1 d
Report 1 X024120.09+001903.1 chandra ccd2 344.167 852.167 2.87049 1.73205 0.0025237 0.0015228 8.96723 0.999834 0.824483 0.492 156.576 8.83304 A F 2.93e+20 0 1 d
Report srcpi bgdpi arf 4 X024136.65+002712.3 chandra ccd7 879.5 656.5 2.69472 1.73206 0.00236917 0.00152281 6.38446 0.999175 0.521845 0.492 2.35031e-08 3.54276 F F 3.02e+20 1.28122e-14 1 dx

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