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 X123049.15+122329.0 chandra ccd7 110.591 839.083 824.324 40.9354 0.176816 0.00878058 28.6091 1 1.49 1.49 0 0.113921 T F 1.94e+20 1.34724e-12 1 dscxf
Report srcpi bgdpi arf rmf 2 X123048.84+122330.1 chandra ccd7 119.284 840.743 115.998 14.4226 0.0248811 0.00309361 4.02583 0.999961 0.492 0.492 123.95 0.149711 F F 1.94e+20 1.80175e-13 1 dbcx
Report srcpi bgdpi arf rmf 3 X123048.63+122332.3 chandra ccd7 126.219 845.828 1019.07 42.4859 0.218589 0.00911319 35.368 1 0.482758 0.482758 0 0.188474 F F 1.93e+20 1.58213e-12 1 dsx
Report srcpi bgdpi arf rmf 4 X123048.19+122335.7 chandra ccd7 139.302 852.69 263.981 25.3887 0.0566234 0.00544582 9.16176 1 1.5 1.5 0 0.27616 T F 1.93e+20 4.09926e-13 1 dsx
Report srcpi bgdpi arf rmf 6 X123049.38+122328.3 chandra ccd7 103.751 837.696 8376.53 98.3839 1.79675 0.0211032 290.717 1 0.511526 0.511526 0 0.0963004 F F 1.94e+20 1.30069e-11 1 dscx

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