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 X021433.88+275947.5 chandra ccd3 1043.28 806 38.6922 6.22031 0.0223068 0.00358613 107.972 1 4.18033 4.18033 0 9.74337 F F 6.09e+20 0 1 ds
Report 3 X021404.09+275239.7 chandra ccd7 719.5 728.375 7.88516 2.82843 0.00454593 0.00163064 14.3021 1 0.57546 0.492 47.5003 2.30621 F F 5.85e+20 0 1 d
Report 1 X021424.07+280645.9 chandra ccd2 582.625 876.5 7.48316 2.82844 0.00431417 0.00163064 21.7787 1 1.77995 0.492 109.466 13.7367 A F 6.17e+20 0 1 d
Report 1 X021411.73+275528.5 chandra ccd7 513.833 1071.5 2.94425 1.73205 0.00169741 0.000998558 5.34028 0.999721 0.492 0.492 180 3.40475 F F 5.94e+20 0 1 d
Report 1 X021334.48+275637.3 chandra ccd6 819 445.5 1.97365 1.41421 0.00113784 0.000815319 5.56435 0.999698 0.492 0.492 63.4349 5.48176 F F 5.84e+20 0 1 d
Report 2 X021420.94+275444.1 chandra ccd7 265.5 981.5 0.989724 1 0.000570593 0.000576517 1.79516 0.962179 0.492 0.492 90 5.27238 F F 5.96e+20 0 1 d

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