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 rmf 1 X132938.62+582505.5 chandra ccd7 137.455 743.977 4321.23 67.2813 0.450885 0.00702026 301.407 1 0.401599 0.401599 0 0.560769 F T 1.75e+20 2.2277e-12 1 dsxf
Report srcpi bgdpi arf 1 X132956.21+583444.2 chandra ccd6 76.3333 893.722 13.8502 4.2427 0.00144515 0.00044269 16.3525 1 2.70693 2.03777 74.0869 9.38686 F T 1.77e+20 1.49721e-14 1 dx
Report srcpi bgdpi arf 2 X132950.93+583322.5 chandra ccd6 160.167 727.767 13.6428 3.87301 0.00142351 0.000404116 16.1077 1 1.78938 0.722682 130.36 7.9205 A F 1.76e+20 1.42853e-14 1 dx
Report srcpi bgdpi arf 3 X132945.40+583008.3 chandra ccd6 247.9 332.9 4.81416 2.23607 0.000502317 0.000233315 5.68394 0.999897 0.764091 0.492 83.7963 4.61178 A F 1.76e+20 4.71462e-15 1 dx

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