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 rmf 3 X193240.51+382534.7 chandra ccd7 534.998 418.975 268.871 16.6912 0.0989534 0.0061429 86.2233 1 0.45122 0.45122 0 0.451262 F F 1.48e+21 9.30005e-13 1 dsxf
Report srcpi bgdpi arf 1 X193151.82+381614.7 chandra ccd2 789.136 559.5 9.24731 3.31667 0.00340344 0.00122069 20.7485 1 4.42372 3.16568 138.371 13.0894 F F 1.44e+21 4.78845e-14 1 dx
Report srcpi bgdpi arf 2 X193239.41+381929.7 chandra ccd6 945 639.667 5.88366 2.44949 0.0021654 0.000901499 12.9709 1 0.55163 0.492 69.0064 5.64302 F F 1.5e+21 2.51754e-14 1 dx
Report 1 X193155.79+382601.2 chandra ccd3 235.5 770.5 2.95596 1.73205 0.0010892 0.000638217 6.39744 0.999927 0.799484 0.492 85.2688 8.86469 A F 1.4e+21 0 1 d
Report srcpi bgdpi arf 1 X193258.63+382321.3 chandra ccd6 485.5 1110.5 1.98474 1.41421 0.000730456 0.000520481 4.3755 0.998755 0.521845 0.492 45 3.91478 F F 1.52e+21 8.03866e-15 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