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 X191226.42+165703.5 chandra ccd6 602.5 708.833 2.99891 1.73205 0.00205895 0.00118917 10.7729 0.999999 0.492 0.492 90 6.15747 F F 6.22e+21 0 1 d
Report 3 X191219.06+170258.2 chandra ccd7 113.167 723.833 2.98712 1.73205 0.00205086 0.00118917 6.11407 0.999888 0.543766 0.492 145.278 3.67114 F F 6.04e+21 0 1 d
Report srcpi bgdpi arf 1 X191207.34+170404.5 chandra ccd7 454.833 858.5 2.93961 1.73205 0.00201824 0.00118917 6.01683 0.999888 0.550073 0.492 108.435 3.17013 F F 5.96e+21 2.08743e-14 1 dx
Report srcpi bgdpi arf 1 X191119.00+164923.5 chandra ccd0 696.5 1315.5 2 1.41421 0.00137314 0.000970954 7.90128 0.999958 1.33045 0.492 56.3099 16.1545 A F 5.79e+21 4.48153e-14 1 dx
Report srcpi bgdpi arf 2 X191211.02+170428.6 chandra ccd7 347.5 907.5 1.97715 1.41421 0.00135745 0.000970954 4.04684 0.998103 0.492 0.492 180 3.73458 F F 5.97e+21 1.41813e-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