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 3 X173203.09+611752.0 chandra ccd7 311.331 821.769 119.002 11.3458 0.0377124 0.00359557 38.1577 1 0.40265 0.317851 102.803 0.296774 F F 3.3e+20 2.55017e-13 1 dsxf
Report srcpi bgdpi arf 1 X173315.31+611906.8 chandra ccd2 917 395.857 12.4096 3.74168 0.00393265 0.00118576 23.9167 1 2.69989 1.86914 106.714 8.80443 F F 3.4e+20 5.44259e-14 1 dx
Report srcpi bgdpi arf 1 X173215.66+612706.3 chandra ccd6 402.722 941.056 7.86509 3.00002 0.00249249 0.000950722 14.0512 1 3.36784 1.32515 71.2476 9.09403 A F 3.26e+20 2.99313e-14 1 dx
Report srcpi bgdpi arf 1 X173145.79+611234.3 chandra ccd7 564.786 175.643 6.72377 2.64576 0.00213079 0.000838453 2.15596 0.978426 0.727721 0.504026 20.8648 5.92627 F F 3.3e+20 1.67819e-14 1 dx
Report srcpi bgdpi arf 1 X173313.13+611125.3 chandra ccd3 671.75 427.75 3.74865 2.00001 0.00118797 0.000633812 7.03549 0.999988 1.67844 0.879828 89.284 10.8463 A F 3.45e+20 1.61815e-14 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