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 1 X123049.06+122329.7 chandra ccd7 179.703 690.269 370.356 32.7964 0.079151 0.00700912 12.5736 1 1.5 1.5 0 0.292432 T F 1.94e+20 5.20487e-13 1 dscxf
Report srcpi bgdpi arf rmf 2 X123048.84+122331.3 chandra ccd7 186.297 693.534 197.425 30.7063 0.0421928 0.00656242 6.70258 1 1.5 1.5 0 0.284639 T F 1.94e+20 3.08361e-13 1 dbcsx
Report srcpi bgdpi arf rmf 3 X123048.63+122332.4 chandra ccd7 192.568 695.656 948.633 41.4004 0.202738 0.00884792 32.2061 1 0.482344 0.482344 0 0.274637 F F 1.93e+20 1.48144e-12 1 dscx
Report srcpi bgdpi arf rmf 4 X123048.24+122335.0 chandra ccd7 204.325 701.099 103.257 26.4864 0.0220676 0.00566056 3.50558 0.999702 1.01855 0.589754 340.974 0.292974 T F 1.93e+20 1.61452e-13 1 dsx
Report srcpi bgdpi arf rmf 8 X123049.39+122328.3 chandra ccd7 170.047 687.343 6079.17 87.1943 1.29921 0.0186348 206.388 1 0.514438 0.514438 0 0.329644 F F 1.94e+20 9.49057e-12 1 dsx

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