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 1 X103231.86+054100.0 chandra ccd7 1064.64 900.643 9.93161 4.27872 0.00645878 0.00278256 37.9768 1 0.609044 0.492 131.015 4.40196 8 1.93161 -0.611018 0.509348 F F 2.8e+20 6.14368e-14 1 dx
Report srcpi bgdpi arf 2 X103255.33+053648.7 chandra ccd7 352.5 389.7 4.94398 3.39792 0.0032152 0.00220975 20.8891 1 0.743448 0.492 8.4292 4.89235 2.94398 2 -0.190936 0.710319 A T 2.81e+20 2.67875e-14 1 dx
Report srcpi bgdpi arf 3 X103249.91+054118.4 chandra ccd7 517.54 938.533 25.8788 5.68879 0.0168302 0.00369968 10.1634 1 0.0893532 0.0893532 0 0.203147 8.65438 1 -0.79284 0.570593 F F 2.8e+20 1.25811e-13 1 dsx

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