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 4 X080405.86+050649.8 chandra ccd7 197.885 245.347 1863.58 44.1903 0.190233 0.00451092 274.411 1 0.448327 0.41547 331.667 0.273933 F F 3.45e+20 6.68611e-12 1 dsxf
Report srcpi bgdpi arf 2 X080405.98+051033.7 chandra ccd7 193.75 700.033 58.7066 7.74598 0.00599272 0.000790704 8.6445 1 0.780299 0.494798 30.3886 3.92356 A F 3.48e+20 4.63129e-14 1 dpx
Report srcpi bgdpi arf 1 X080403.50+050748.6 chandra ccd7 269.458 364.824 21.5353 4.95719 0.00219831 0.000506026 3.17106 0.998489 0.452509 0.452509 0 1.40757 F F 3.45e+20 1.62013e-14 1 dsx
Report srcpi bgdpi arf 1 X080409.05+050414.7 chandra ccd6 389.987 912.149 21.1735 4.60809 0.00216138 0.000470391 21.4162 1 0.968684 0.520671 77.6469 2.47243 T F 3.43e+20 2.20883e-14 1 dsx

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