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 X002839.71+003540.0 chandra ccd2 520.431 287.259 115.791 11.9584 0.0743386 0.00767734 150.911 1 1.02072 0.71628 151.261 11.3468 F F 2.75e+20 0 1 d
Report 2 X002752.41+002615.1 chandra ccd7 981.786 447.435 7.81943 2.79632 0.0247491 0.00885058 7.04977 0.999999 0.865395 0.865395 0 4.48632 F F 2.64e+20 0 1 ds
Report 1 X002756.85+003048.0 chandra ccd7 846.062 1001.75 13.386 4.00004 0.00859386 0.00256804 12.0684 1 0.689409 0.492 122.397 0.806854 T F 2.67e+20 0 1 db
Report 1 X002808.00+003528.6 chandra ccd6 145.1 574.1 4.89397 2.23607 0.00314195 0.00143557 5.64015 0.999867 0.768298 0.492 99.645 5.52665 A F 2.71e+20 0 1 d
Report 2 X002752.13+003822.6 chandra ccd6 629.1 927.7 4.67194 2.23608 0.0029994 0.00143557 5.38426 0.999867 0.492 0.492 59.8724 8.22259 F F 2.7e+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