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 1 X105752.85+440259.7 chandra ccd7 104.833 470.167 5.76979 3.59808 0.00392888 0.00245007 12.0254 1 1.28761 0.700263 105.609 6.88495 2.95396 2.81583 -0.0239394 0.63205 A F 8.63e+19 3.33285e-14 1 dx
Report 3 X105720.80+440040.5 chandra ccd7 807.1 186.5 4.97793 2.23607 0.00338967 0.00152263 12.4346 1 0.50423 0.492 7.76206 2.7901 F F 8.74e+19 0 1 d
Report 2 X105737.46+440214.9 chandra ccd7 441.9 378.5 4.9533 2.23607 0.0033729 0.00152263 12.3731 1 0.645911 0.492 108.264 4.23222 F F 8.68e+19 0 1 d
Report srcpi bgdpi arf 1 X105632.51+435720.8 chandra ccd6 899.833 137.5 2.9711 2.93649 0.00202314 0.00199957 17.4776 1 1.44155 0.492 170.917 9.5803 1 1.9711 0.326849 1.06229 A F 9.12e+19 2.68484e-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