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 X131327.19-271923.9 chandra ccd7 776.155 172.026 14.6118 6.53361 0.000798379 0.000356992 2.83797 0.996705 0.796185 0.796185 0 5.40531 F F 5.94e+20 6.28953e-15 1 dsx
Report srcpi bgdpi arf 2 X131328.82-271914.5 chandra ccd7 732.116 190.968 31.9909 6.45496 0.00174796 0.000352695 6.21341 1 1.63877 0.817645 89.6477 5.01433 F F 5.93e+20 1.3684e-14 1 dsx
Report srcpi bgdpi arf rmf 3 X131347.38-271649.2 chandra ccd7 229.414 486.601 897.901 30.8765 0.0490608 0.00168708 174.394 1 0.396579 0.396579 0 0.289747 F F 5.89e+20 3.59735e-13 1 dsxf
Report srcpi bgdpi arf 5 X131346.57-271652.3 chandra ccd7 251.338 480.348 18.0648 5.55786 0.000987048 0.000303678 3.50863 0.999338 0.384519 0.384519 0 0.426683 F F 5.89e+20 8.22905e-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