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 3 X022600.32-152028.7 chandra ccd7 913.86 848.099 435.304 21.5229 0.149111 0.00737257 116.479 1 0.44389 0.38965 30.4863 0.599261 F F 1.84e+20 6.16694e-13 1 dsxf
Report srcpi bgdpi arf 1 X022559.57-152023.3 chandra ccd7 935.889 859.147 33.4846 5.78663 0.01147 0.00198218 8.95985 1 0.471723 0.471723 0 0.430262 F F 1.84e+20 8.03489e-14 1 dsx
Report srcpi bgdpi arf 1 X022633.04-150924.4 chandra ccd2 267.134 633.042 13.3228 5.56016 0.00456367 0.00190461 3.17637 0.997599 4.69234 4.69234 0 13.4481 F F 1.88e+20 6.27731e-14 1 dsx
Report srcpi bgdpi arf 1 X022637.79-151700.4 chandra ccd3 838.389 448.722 7.5165 3.00003 0.00257471 0.00102763 17.2677 1 3.01954 1.64003 126.327 9.84829 A F 1.92e+20 3.58897e-14 1 dx
Report srcpi bgdpi arf 1 X022551.29-151332.3 chandra ccd6 383 960 1.96305 1.41421 0.000672424 0.000484426 4.68576 0.99921 0.492 0.492 45 6.70747 F F 1.79e+20 7.98515e-15 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