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 1 X141951.22+113525.4 chandra ccd7 369.012 624.604 24.0756 4.90669 0.0158099 0.0032221 49.5806 1 0.686866 0.686866 0 3.54893 F F 1.95e+20 1.17529e-13 1 dsx
Report srcpi bgdpi arf 1 X141925.33+112830.9 chandra ccd6 997.722 811.722 8.63526 3.00001 0.00567039 0.00196997 28.5967 1 1.33014 0.798705 12.2924 5.97472 A F 1.96e+20 7.03496e-14 1 dx
Report srcpi bgdpi arf 2 X141924.74+112658.1 chandra ccd6 1015.62 623.125 7.76714 2.82843 0.00510033 0.00185731 25.7218 1 1.19153 0.858808 173.329 7.15968 F F 1.97e+20 6.80312e-14 1 dx
Report 3 X141948.44+113309.8 chandra ccd7 451.5 348.5 3.96204 2 0.00260169 0.00131331 8.15931 0.999995 0.492 0.492 90 1.34921 F F 1.96e+20 0 1 d
Report srcpi bgdpi arf 2 X141946.66+113553.5 chandra ccd7 504.5 681.167 2.96794 1.73205 0.00194891 0.00113736 6.11208 0.999893 0.492 0.492 90 3.61501 F F 1.95e+20 1.44493e-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