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 X191211.60+165716.8 chandra ccd2 1144.1 482.5 4.81991 2.23608 0.00330919 0.00153522 18.9907 1 0.492 0.492 3.39659e-08 15.5225 F F 6.08e+21 0 1 d
Report 1 X191213.00+170343.5 chandra ccd3 374.75 479.5 3.67704 2.00001 0.00252454 0.00137314 14.0146 0.999999 1.92963 1.53662 45.895 10.5641 F F 5.99e+21 0 1 d
Report 1 X191258.72+170749.2 chandra ccd6 832.167 941.5 2.99613 1.73205 0.00205705 0.00118917 11.0872 0.999999 0.492 0.492 40.2688 3.36866 F F 6.27e+21 0 1 d
Report 1 X191242.18+170846.3 chandra ccd7 653.167 345.5 2.9544 1.73205 0.0020284 0.00118917 5.83481 0.999853 0.627179 0.492 56.3099 1.96635 F F 6.14e+21 0 1 d
Report 2 X191209.79+170104.0 chandra ccd3 468.5 155.5 1.99621 1.41421 0.00137053 0.000970954 7.60828 0.999948 1.16688 0.492 161.565 12.8845 A F 5.99e+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