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 arf 1 X043939.52+071654.9 chandra ccd2 416.5 992.786 6.94684 2.64575 0.00820421 0.00312463 30.6394 1 1.25712 0.594716 29.4513 6.98216 A F 9.02e+20 9.01553e-14 1 dx
Report arf 1 X043906.90+071702.3 chandra ccd3 445 620.75 3.96381 2 0.00468126 0.002362 9.37393 0.999999 0.497677 0.492 70.6701 3.16485 F F 9.16e+20 4.71936e-14 1 dx
Report 1 X043921.87+070656.0 chandra ccd0 587 675.5 1.98719 1.41421 0.00234687 0.00167019 9.0162 0.999982 0.665224 0.492 33.6901 7.67398 F F 9.05e+20 0 1 d
Report arf 1 X043953.75+072739.2 chandra ccd6 595.5 1121.5 0.999988 1 0.00118099 0.001181 4.28435 0.998569 0.492 0.492 90 16.6764 F F 9.14e+20 1.50396e-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