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 X160157.74+380901.6 chandra ccd7 931.625 483.875 7.9696 2.82843 0.00773754 0.00274607 17.9955 1 0.492 0.492 23.6453 2.29146 F F 1.37e+20 0 1 d
Report srcpi bgdpi arf 3 X160207.65+380743.1 chandra ccd7 694 324.167 5.96758 2.44949 0.00579383 0.00237817 13.4749 1 0.492 0.492 158.085 0.107133 F F 1.36e+20 4.16406e-14 1 dx
Report 2 X160203.48+380702.9 chandra ccd7 794.167 242.5 2.98402 1.73205 0.00289714 0.00168162 6.73799 0.999947 0.492 0.492 90 0.957175 F F 1.37e+20 0 1 d
Report 1 X160205.05+380540.1 chandra ccd6 439.5 1019.17 2.96998 1.73205 0.00288351 0.00168162 10.6713 0.999999 0.561105 0.492 154.903 2.04989 F F 1.38e+20 0 1 d
Report srcpi bgdpi arf 1 X160046.00+380616.1 chandra ccd2 1076.83 551.833 2.69355 1.73207 0.00261512 0.00168164 10.3684 0.999951 3.60411 0.828853 14.7326 16.0235 A F 1.46e+20 3.97999e-14 1 dx
Report srcpi bgdpi arf 2 X160106.07+380230.6 chandra ccd2 596.643 91.9285 6.1803 2.64578 0.00600035 0.00256874 23.7901 1 3.89164 1.08012 169.529 13.0828 A F 1.46e+20 9.23112e-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