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 3 X101956.61+274401.9 chandra ccd7 933.891 494.657 15.8717 3.98393 0.0108078 0.00271285 38.7301 1 0.614457 0.287621 42.7537 0.184507 8 4.88105 -0.242135 0.378748 F F 2.5e+20 8.1009e-14 1 dsx
Report srcpi bgdpi arf 1 X101918.49+273933.0 chandra ccd6 883.75 247.375 7.86366 3.95804 0.00535468 0.00269519 21.2963 1 3.30657 0.760626 168.817 9.41824 3.98052 3.88313 -0.0123847 0.508708 A F 2.46e+20 6.75802e-14 1 dx
Report srcpi bgdpi arf 2 X102001.58+274526.9 chandra ccd7 799.3 667.1 4.83061 3.39792 0.00328936 0.00231378 11.7372 1 0.492 0.492 114.699 1.97062 4.83061 0 -1 1.00987 F F 2.51e+20 2.47433e-14 1 dx
Report 1 X101953.63+274128.5 chandra ccd7 1013.83 182.5 2.98161 1.73205 0.0020303 0.00117942 7.27572 0.999971 0.492 0.492 180 2.45583 F F 2.49e+20 0 1 d
Report srcpi bgdpi arf 2 X101932.82+274251.2 chandra ccd6 496.5 649.833 3.96578 3.17945 0.00270046 0.00216501 21.4369 1 1.21764 0.492 90 5.29846 2 1.96578 -0.00862989 0.816029 A F 2.48e+20 3.36602e-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