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 X123049.16+122328.9 chandra ccd7 108.595 837.242 856.736 44.801 0.182166 0.00952592 24.3087 1 1.5 1.5 0 0.118765 T F 1.94e+20 1.34504e-12 1 dscxf
Report srcpi bgdpi arf rmf 2 X123048.99+122329.2 chandra ccd7 113.616 837.871 488.782 39.8166 0.103928 0.0084661 13.8685 1 1.5 1.5 0 0.148104 T F 1.94e+20 7.52547e-13 1 dbcsx
Report srcpi bgdpi arf rmf 3 X123048.63+122332.4 chandra ccd7 124.486 844.299 948.716 42.5209 0.201723 0.00904112 26.9185 1 0.494982 0.494982 0 0.193254 F F 1.93e+20 1.46026e-12 1 dsx
Report srcpi bgdpi arf 5 X123048.22+122335.1 chandra ccd7 136.664 849.968 92.4999 23.8816 0.019668 0.00507788 2.62456 0.995253 0.812192 0.812192 0 0.284094 F F 1.93e+20 1.42385e-13 1 dsx
Report srcpi bgdpi arf rmf 7 X123049.38+122328.3 chandra ccd7 102.224 836.163 8491.4 105.442 1.80551 0.0224198 240.932 1 0.505466 0.505466 0 0.101087 F F 1.94e+20 1.3074e-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