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 X135419.96+325547.8 chandra ccd7 306.358 267.677 1681.25 42.0711 0.1769 0.0044267 301.185 1 0.415302 0.415302 0 0.565069 F T 1.32e+20 0 1 ds
Report 2 X135404.74+325541.5 chandra ccd7 695.915 254.996 10.0495 3.84707 0.0010574 0.000404785 1.8003 0.963303 0.681207 0.681207 0 3.75933 F F 1.33e+20 0 1 ds
Report 3 X135351.87+325546.2 chandra ccd7 1024.67 264.333 12.6344 3.87304 0.00132939 0.000407519 2.26337 0.982691 0.511611 0.492 72.0812 6.45887 F F 1.34e+20 0 1 d
Report 4 X135400.86+325541.9 chandra ccd7 794.625 255.5 12.3496 3.60556 0.00129941 0.000379375 2.21234 0.982691 0.492 0.492 90 4.57319 F F 1.33e+20 0 1 d
Report 5 X135422.53+325522.1 chandra ccd7 240.695 215.461 70.4649 8.39434 0.00741428 0.000883248 12.6233 1 0.456844 0.456844 0 0.411223 F F 1.32e+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