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 X134859.45+601458.0 chandra ccd7 367.268 668.008 253.893 16.475 0.0184421 0.00119669 51.0409 1 0.922248 0.922248 0 4.09607 F F 1.64e+20 0 1 ds
Report 2 X134915.95+601127.9 chandra ccd7 117.167 240.405 18.7338 4.58261 0.00136077 0.000332867 3.76612 0.999701 0.642341 0.492 47.3234 0.211056 T F 1.64e+20 0 1 dbp
Report 3 X134915.28+601126.3 chandra ccd7 127.738 237.636 110.34 12.6884 0.00801474 0.000921646 22.182 1 1.46502 1.46502 0 0.129504 T F 1.64e+20 0 1 ds
Report 5 X134913.11+601122.6 chandra ccd7 160.697 229.979 13.2409 4.39138 0.000961779 0.000318977 2.66186 0.992077 0.337592 0.337592 0 0.195627 F F 1.64e+20 0 1 ds

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