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 1 X063921.67+051642.1 chandra ccd7 393.667 479.167 5.92508 2.44949 0.00160718 0.000664425 7.89958 0.999998 0.492 0.492 5.39215 2.30756 F F 5.97e+21 0 1 d
Report srcpi bgdpi arf 2 X063918.19+051534.5 chandra ccd7 499.333 341.667 5.87656 2.44949 0.00159402 0.000664425 7.8349 0.999998 0.61656 0.492 20.3661 2.07722 F F 5.97e+21 1.58042e-14 1 dx
Report srcpi bgdpi arf 3 X063925.55+052102.8 chandra ccd7 276.307 1009.47 16.0006 4.00007 0.00434017 0.00108502 21.3327 1 1.40734 1.40734 0 6.43773 F F 5.96e+21 4.85824e-14 1 dsx
Report srcpi bgdpi arf 4 X063925.67+051430.2 chandra ccd7 272.909 211.466 31.1389 5.58022 0.00844644 0.00151364 41.5158 1 0.373674 0.373674 0 0.108952 F F 5.97e+21 8.34532e-14 1 dsx

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