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 2 X094740.91+142515.2 chandra ccd7 552.928 851.214 6.8736 3.78388 0.00441384 0.0024298 19.3338 1 0.659721 0.492 168.125 4.38324 5 1 -0.666667 0.730275 F F 3.06e+20 3.4432e-14 1 dx
Report srcpi bgdpi arf 1 X094746.97+142624.3 chandra ccd7 374.167 991.667 5.92578 3.59808 0.0038052 0.00231048 21.751 1 1.12287 0.492 97.3015 6.04771 5 1.92578 -0.443881 0.60479 A F 3.06e+20 3.069e-14 1 dx
Report 1 X094730.27+141819.8 chandra ccd6 446.25 981 3.98472 2 0.00255876 0.00128429 13.6737 1 0.534007 0.492 133.977 3.00383 F F 3.05e+20 0 1 d
Report 3 X094734.20+142117.0 chandra ccd7 751.25 367 3.96436 2 0.00254569 0.00128429 9.56885 0.999999 0.492 0.492 52.0181 0.193451 F F 3.05e+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