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 198.837 252.349 1826.23 43.7662 0.194024 0.00464986 308.543 1 0.439182 0.439182 0 0.27369 F F 3.45e+20 6.80368e-12 1 dsxf
Report srcpi bgdpi arf 2 X080405.95+051034.2 chandra ccd7 196.013 708.47 65.2937 8.85642 0.00693698 0.000940929 11.0314 1 0.852994 0.852994 0 3.93122 F F 3.48e+20 5.3528e-14 1 dsx
Report srcpi bgdpi arf 1 X080403.51+050748.7 chandra ccd7 270.078 371.984 19.1479 4.67453 0.00203433 0.000496635 3.23505 0.998911 0.413453 0.413453 0 1.40733 F F 3.45e+20 1.5012e-14 1 dsx
Report srcpi bgdpi arf 3 X080358.94+051138.8 chandra ccd7 408.25 839.25 13.2506 4.00004 0.00140778 0.000424974 2.2387 0.985202 2.2535 0.592591 176.796 5.36005 A F 3.48e+20 1.11902e-14 1 dx
Report srcpi bgdpi arf 1 X080409.05+050415.0 chandra ccd6 376.958 931.781 11.65 3.41321 0.00123773 0.000362628 11.5654 1 0.971332 0.500774 87.5534 2.46594 F F 3.43e+20 1.26427e-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