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 X011058.91+330906.9 chandra ccd7 527.926 339.583 65.8874 12.0554 0.0257775 0.00471651 7.39207 1 0.870611 0.870611 0 0.991595 T F 5.45e+20 1.81726e-13 1 dsx
Report 1 X011107.74+330449.6 chandra ccd6 249.875 851.25 7.91202 2.82843 0.00309545 0.00110658 18.6189 1 0.823585 0.492 96.1876 3.84079 A F 5.49e+20 0 1 d
Report 2 X011056.08+330410.1 chandra ccd6 547.75 770.75 3.94356 2 0.00154285 0.000782467 9.28015 0.999999 0.589598 0.492 123.019 3.99183 F F 5.48e+20 0 1 d
Report 3 X011043.20+330148.2 chandra ccd6 876.833 482.5 2.96404 1.73205 0.00115963 0.000677637 6.97509 0.999962 0.492 0.492 180 7.08068 F F 5.48e+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