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 rmf 1 X100120.68+555355.6 chandra ccd7 663.028 339.144 246.076 16.3966 0.0791914 0.00527671 61.1171 1 0.405622 0.405622 0 0.390974 F F 9.29e+19 5.98728e-13 1 dsxf
Report srcpi bgdpi arf rmf 2 X100120.82+555349.6 chandra ccd7 660.573 326.916 223.42 15.2666 0.0719003 0.00491305 55.4901 1 0.418039 0.418039 0 0.291318 F F 9.29e+19 5.35425e-13 1 dsx
Report srcpi bgdpi arf 1 X100059.55+555140.5 chandra ccd6 382.593 847.709 16.412 4.05117 0.00528167 0.00130374 35.7735 1 1.11807 1.11807 0 3.49302 F F 9.28e+19 5.79755e-14 1 dsx
Report srcpi bgdpi arf 2 X100113.95+554955.3 chandra ccd6 135.75 633.25 3.94187 2 0.00126855 0.000643629 8.59215 0.999997 0.704338 0.492 139.213 3.73463 F F 9.27e+19 1.40389e-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