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 X132938.61+582505.7 chandra ccd7 416.557 635.35 595.552 24.6441 0.115812 0.00479234 226.674 1 1.25447 0.663286 356.785 4.22986 A F 1.75e+20 4.80478e-13 1 dsxf
Report srcpi bgdpi arf 2 X132956.18+582220.8 chandra ccd7 136.047 299.987 18.7433 4.88371 0.00364485 0.000949694 7.13391 1 0.377755 0.377755 0 0.807375 F F 1.76e+20 2.45611e-14 1 dsx
Report srcpi bgdpi arf 4 X132955.08+582151.4 chandra ccd7 153.634 240.357 10.8149 3.82582 0.00210309 0.000743976 4.11627 0.999692 0.349801 0.349801 0 0.345602 F F 1.7e+20 1.40933e-14 1 dsx
Report srcpi bgdpi arf 1 X133025.85+581558.9 chandra ccd6 247.722 352.722 8.37435 3.00001 0.00162849 0.000583387 13.5816 1 1.2785 0.53713 4.23708 6.79413 A F 1.69e+20 1.73029e-14 1 dx
Report srcpi bgdpi arf 3 X132940.07+582454.2 chandra ccd7 392.786 611.357 6.58774 2.64576 0.00128106 0.000514498 2.50737 0.988509 0.738317 0.492 170.891 3.9651 A F 1.75e+20 9.03177e-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