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 4 X131914.24+520200.3 chandra ccd7 378.944 780.611 8.95734 3 0.00580896 0.00194554 20.4394 1 0.492 0.492 172.534 0.188013 F F 1.34e+20 0 1 d
Report srcpi bgdpi arf 2 X131909.87+520519.3 chandra ccd7 460.833 1185 6.91531 3.78388 0.00448468 0.0024539 23.7622 1 0.492 0.492 3.03638e-08 3.21231 5 2 -0.428571 0.595029 F F 1.34e+20 3.79476e-14 1 dx
Report srcpi bgdpi arf 1 X131854.81+520300.6 chandra ccd7 743.333 903.333 5.92294 3.59808 0.00384111 0.0023334 21.3361 1 0.541108 0.492 85.2688 3.1383 5 1 -0.666667 0.730275 F F 1.35e+20 3.23901e-14 1 dx
Report srcpi bgdpi arf 3 X131854.45+520218.6 chandra ccd7 750.1 817.9 4.84954 3.39792 0.003145 0.0022036 12.5022 1 0.553834 0.492 85.4549 3.08644 5 0 -1 0.975663 F F 1.35e+20 2.42098e-14 1 dx
Report 1 X131943.93+520555.7 chandra ccd6 764.833 834.5 2.974 1.73205 0.00192868 0.00112326 10.6558 0.999999 0.492 0.492 161.565 5.86846 F F 1.33e+20 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