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 X191121.77+164830.0 chandra ccd6 957.167 1088.5 2.9794 1.73205 0.00205001 0.00119176 10.7195 0.999999 0.492 0.492 5.35186e-08 2.2731 F F 5.82e+21 0 1 d
Report 1 X191052.69+165310.0 chandra ccd7 1068.5 900.833 2.96841 1.73205 0.00204244 0.00119176 6.47788 0.999931 0.54799 0.492 123.019 6.11466 F F 5.56e+21 0 1 d
Report 3 X191100.34+165131.2 chandra ccd7 845.5 699.833 2.9623 1.73205 0.00203824 0.00119176 6.46454 0.999931 0.510281 0.492 61.845 3.6789 F F 5.63e+21 0 1 d
Report 2 X191104.62+164644.2 chandra ccd7 720.5 116.5 0.991834 1 0.000682442 0.000688061 2.16446 0.98081 0.492 0.492 90 3.57122 F F 5.71e+21 0 1 d

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