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 X060731.79+222126.6 chandra ccd5 484.286 588.124 1389.78 39.3864 0.281614 0.00798096 109.358 1 12.4096 9.56694 12.8767 14.8209 F F 4.31e+21 2.39127e-12 1 dsxf
Report srcpi bgdpi arf rmf 3 X060726.62+220547.6 chandra ccd7 484.928 744.698 296.425 17.5665 0.060065 0.00355953 85.013 1 0.462537 0.374669 345.702 0.996317 F F 4.44e+21 1.57425e-12 1 dsxf
Report srcpi bgdpi arf 1 X060732.71+221104.6 chandra ccd6 387.036 357.019 16.7271 4.66918 0.00338944 0.000946123 7.42575 1 1.36773 0.629827 27.1494 4.72557 F F 4.39e+21 4.2978e-14 1 dsx
Report srcpi bgdpi arf 1 X060714.80+220329.3 chandra ccd7 818.375 463.125 7.8298 2.82843 0.00158655 0.000573124 2.24554 0.976053 0.555946 0.492 80.0724 3.9866 F F 4.45e+21 1.53886e-14 1 dx
Report srcpi bgdpi arf 2 X060732.51+220036.6 chandra ccd7 318 112.125 7.15737 2.82844 0.0014503 0.000573127 2.05269 0.976053 1.31532 0.717261 66.0458 6.34717 A F 4.49e+21 1.48807e-14 1 dx
Report srcpi bgdpi arf 10 X060727.49+220447.8 chandra ccd7 459.928 622.643 6.87702 2.64575 0.00139349 0.000536109 1.97229 0.976053 0.492 0.492 157.5 2.00271 F F 4.45e+21 1.30657e-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