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 X045549.90+453353.7 chandra ccd6 605.071 197.786 6.91823 2.64575 0.00236797 0.000905586 21.1212 1 0.614776 0.492 44.3014 2.6616 F F 5.51e+21 2.90575e-14 1 dx
Report srcpi bgdpi arf 2 X045707.85+452754.5 chandra ccd3 605.75 57.25 3.57142 2.00001 0.00122244 0.000684571 11.6002 0.999997 1.0278 0.492 46.8759 12.5028 A F 5.47e+21 3.31385e-14 1 dx
Report 1 X045702.91+453110.2 chandra ccd3 712.5 454.5 1.99991 1.41421 0.000684538 0.000484062 6.49582 0.999868 1.52143 0.492 14.0362 10.9867 A F 5.44e+21 0 1 d
Report 1 X045635.10+453703.7 chandra ccd2 923 254.5 1.99999 1.41421 0.000684525 0.000484035 6.76364 0.999896 0.665224 0.492 146.31 7.93575 F F 5.41e+21 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