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 1 X084831.65-694105.5 chandra ccd7 824.164 434.637 211.866 14.8688 0.105402 0.0073971 69.7979 1 0.388488 0.388488 0 0.288335 F F 6.39e+20 8.80956e-13 1 dsxf
Report srcpi bgdpi arf rmf 1 X084739.53-694926.3 chandra ccd6 846.207 305.823 135.693 11.6487 0.0675061 0.00579515 313.431 1 5.72928 3.98952 359.615 9.22488 F F 6.63e+20 8.27936e-13 1 dsxf
Report srcpi bgdpi arf 1 X084628.50-695620.8 chandra ccd5 1077.5 389.5 10.6127 4.0001 0.00527972 0.00199001 12.7318 1 5.39486 3.2875 70.9947 18.3464 A F 6.88e+20 6.12667e-14 1 dx
Report 4 X084834.23-694207.1 chandra ccd7 796.357 309.072 6.934 2.64575 0.0034496 0.00131624 2.28436 0.986356 0.492 0.492 79.0993 0.773914 F F 6.39e+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