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 154.135 237.514 1564.17 40.3521 0.159826 0.00412314 328.156 1 0.43135 0.43135 0 0.271486 F F 3.45e+20 4.82219e-12 1 dsxf
Report srcpi bgdpi arf rmf 2 X080405.95+051034.1 chandra ccd7 151.3 693.491 102.532 10.3232 0.0104766 0.00105482 21.5108 1 0.957423 0.957423 0 3.97063 F F 3.48e+20 8.09434e-14 1 dsx
Report srcpi bgdpi arf 1 X080403.51+050748.5 chandra ccd7 225.645 356.838 22.8296 4.77803 0.00233271 0.000488216 4.78955 0.999988 0.429662 0.429662 0 1.41205 F F 3.45e+20 1.71845e-14 1 dsx
Report srcpi bgdpi arf 1 X080406.17+050424.9 chandra ccd6 190.617 985.049 13.4131 3.66239 0.00137054 0.000374219 13.2778 1 0.875921 0.446325 40.9511 2.18572 F F 3.42e+20 1.39757e-14 1 dsx
Report srcpi bgdpi arf 2 X080409.07+050414.8 chandra ccd6 102.724 964.445 11.2792 3.35845 0.0011525 0.000343163 11.1654 1 0.710946 0.376863 251.239 2.44323 F F 3.43e+20 1.1785e-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