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 2 X132938.61+582505.6 chandra ccd7 669.748 389.054 1405.6 37.7227 0.269934 0.00724432 679.91 1 0.944178 0.519507 154.177 4.23428 A T 1.75e+20 0 1 d
Report 1 X132927.74+582534.7 chandra ccd7 843.087 448.63 43.0094 6.78236 0.00825958 0.00130249 20.8043 1 0.812688 0.76796 73.5744 5.72548 F F 1.73e+20 0 1 d
Report 1 X132911.89+581647.5 chandra ccd3 109.355 687.417 36.0334 6.00278 0.00691992 0.00115279 48.4665 1 4.05349 4.05349 0 9.66652 F F 1.63e+20 0 1 ds
Report 3 X132954.41+582406.3 chandra ccd7 417.5 268.333 5.46974 2.4495 0.00105042 0.000470406 2.64579 0.987578 0.492 0.492 150.128 1.94352 F F 1.76e+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