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 X090942.48+044136.8 chandra ccd7 436.685 326.674 13.7709 3.71092 0.00144857 0.000390355 8.89607 1 0.584426 0.584426 0 3.75016 8.746 3.57666 -0.419498 0.417278 F F 3.21e+20 1.11525e-14 1 dsx
Report srcpi bgdpi arf 1 X091013.13+043458.6 chandra ccd3 488.75 445.833 9.82042 4.57071 0.00103302 0.000480797 6.65186 0.999999 1.59562 1.24467 121.304 11.1161 7.14138 2.67904 -0.454394 0.515123 F F 3.21e+20 1.42757e-14 1 dx
Report srcpi bgdpi arf 1 X091003.69+044832.2 chandra ccd6 443.643 373.5 8.5826 4.1225 0.00090281 0.000433649 13.2844 1 0.798944 0.492 38.5625 4.96361 7.73912 0.843475 -0.803445 0.622106 A F 3.28e+20 9.92469e-15 1 dx
Report srcpi bgdpi arf 1 X090947.39+044314.6 chandra ccd7 286.75 525 2.98368 3.17945 0.000313855 0.000334448 2.95963 0.996084 0.492 0.492 29.8718 1.71142 1.83061 1.91531 0.0226095 0.864112 F F 3.22e+20 2.35319e-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