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 3 X122656.46+150250.9 chandra ccd7 566.996 874.061 6.60228 3.78441 0.00741041 0.00424762 2.3763 0.987013 0.3393 0.3393 0 0.555854 F F 2.49e+20 5.01688e-14 1 dsx
Report srcpi bgdpi arf 1 X122715.87+145401.4 chandra ccd3 900.786 675.357 6.50719 2.64576 0.00730346 0.00296952 22.9468 1 2.67853 0.756811 30.1096 10.1856 A F 2.6e+20 1.0078e-13 1 dx
Report 2 X122737.16+145227.3 chandra ccd3 273.5 484.5 0.999758 1 0.0011221 0.00112237 3.52553 0.996935 0.492 0.492 90 14.3475 F F 2.62e+20 0 1 d
Report 1 X122655.14+150758.4 chandra ccd6 1155.5 621.5 0.992337 1 0.00111377 0.00112237 3.66761 0.997448 0.492 0.492 90 4.7709 F F 2.41e+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