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 1 X080342.06+302254.5 chandra ccd7 330.273 857.617 71.2755 8.58116 0.0177635 0.00213862 47.2927 1 0.449688 0.351054 314.699 0.111576 F F 4.06e+20 0 1 ds
Report srcpi bgdpi arf 1 X080402.91+303510.2 chandra ccd5 522.107 418.144 58.1454 12.4873 0.0144912 0.00311211 5.87999 1 7.10062 7.10062 0 12.9747 F F 3.97e+20 1.3603e-13 1 dsx
Report srcpi bgdpi arf 1 X080347.53+302645.3 chandra ccd6 544.585 357.761 24.4662 4.94633 0.00609754 0.00123274 31.6473 1 1.07636 1.07636 0 3.95147 F F 4.03e+20 6.33835e-14 1 dsx
Report srcpi bgdpi arf 3 X080353.18+302446.9 chandra ccd6 395.5 116.625 7.89151 2.82843 0.00196672 0.000704902 10.2078 1 0.492 0.492 90 2.93519 F T 4.02e+20 2.01418e-14 1 dx
Report srcpi bgdpi arf 2 X080349.57+302449.4 chandra ccd6 490.333 121.667 5.90572 2.44949 0.00147183 0.000610463 7.63913 0.999997 0.720336 0.492 148.476 2.41016 T F 4.03e+20 1.49138e-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