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 4 X103426.75+435150.3 chandra ccd7 658.865 263.622 35.0763 6.24099 0.0230337 0.0040983 30.8686 1 0.846525 0.32665 36.92 3.16905 A F 1.14e+20 0 1 ds
Report 1 X103433.02+435154.1 chandra ccd7 521.189 271.365 24.4766 4.94738 0.0160731 0.00324882 21.5404 1 0.826812 0.826812 0 4.00077 F F 1.14e+20 0 1 ds
Report srcpi bgdpi arf 2 X103413.75+435345.9 chandra ccd7 944.778 498.438 17.848 4.22469 0.0117204 0.00277425 15.707 1 0.478295 0.478295 0 0.380423 F F 1.13e+20 8.40188e-14 1 dsx
Report srcpi bgdpi arf 3 X103436.86+435519.6 chandra ccd7 436.667 688.667 5.92536 2.44949 0.00389092 0.00160847 5.21455 0.999939 0.558637 0.492 40.1362 4.19911 F F 1.15e+20 2.87903e-14 1 dx
Report srcpi bgdpi arf 1 X103342.72+435006.4 chandra ccd6 646.667 436.333 5.49782 2.4495 0.00361017 0.00160848 18.5103 1 1.30983 0.953534 8.45258 6.99806 F F 1.11e+20 4.20131e-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