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 4 X024854.25+180249.0 chandra ccd7 187.454 307.555 18.1594 4.26138 0.0104794 0.00245915 31.3838 1 0.392655 0.392655 0 0.610134 F F 8.23e+20 0 1 ds
Report srcpi bgdpi arf 3 X024844.67+180814.0 chandra ccd7 465.014 968.173 16.5665 4.0702 0.00956014 0.00234882 28.6309 1 2.42725 1.4431 359.74 6.45384 F F 8.03e+20 6.50995e-14 1 dsx
Report 1 X024849.85+180423.6 chandra ccd7 314.5 499.25 3.96368 2 0.00228733 0.00115415 6.85019 0.999973 0.492 0.492 28.9973 2.44601 F F 8.16e+20 0 1 d
Report 2 X024846.54+180752.1 chandra ccd7 410.25 923 3.91418 2 0.00225877 0.00115415 6.76466 0.999973 0.699555 0.492 45.651 5.9647 F F 8.05e+20 0 1 d
Report arf 1 X024855.16+175855.1 chandra ccd6 410.5 794.5 0.983569 1 0.000567592 0.000577074 2.58594 0.990492 0.492 0.492 90 3.29618 F F 8.27e+20 5.08775e-15 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