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 X092158.68+505612.5 chandra ccd7 752.975 409.955 17.045 4.12856 0.00974449 0.00236026 30.4002 1 1.41809 0.774529 329.465 4.12358 A F 1.34e+20 5.034e-14 1 dsx
Report srcpi bgdpi arf 3 X092202.23+505854.5 chandra ccd7 684.76 739.293 13.4578 3.66849 0.00769373 0.00209725 24.0023 1 0.635809 0.335549 11.608 1.46692 F T 1.33e+20 4.05652e-14 1 dsx
Report srcpi bgdpi arf 4 X092202.50+505819.3 chandra ccd7 679.072 667.214 6.69485 2.64576 0.00382735 0.00151254 11.9404 1 0.492 0.492 139.731 2.04857 F F 1.33e+20 2.04124e-14 1 dx
Report 2 X092149.06+510213.7 chandra ccd6 576.75 131.75 3.98014 2 0.00227134 0.00114134 12.2031 1 0.492 0.492 90 2.55214 F F 1.32e+20 0 1 d
Report arf 1 X092154.83+510326.9 chandra ccd6 466.167 280.5 2.99315 1.73205 0.00170809 0.000988425 9.17698 0.999995 0.492 0.492 180 3.22023 F F 1.32e+20 1.54133e-14 1 dx
Report arf 1 X092245.76+510250.0 chandra ccd3 1145 946.5 1.9369 1.41422 0.00110535 0.000807067 6.18315 0.999854 0.665224 0.492 146.31 7.63342 F F 1.36e+20 1.80265e-14 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