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 1 X080432.27+650105.0 chandra ccd7 247.071 370.214 6.76083 2.64576 0.00101157 0.000395862 4.31291 0.999758 0.492 0.492 164.71 1.38055 F F 4.17e+20 7.58672e-15 1 dx
Report srcpi bgdpi arf 2 X080414.15+650236.3 chandra ccd7 480.518 556.476 11.2833 3.35906 0.00168823 0.00050259 7.19791 1 0.531548 0.531548 0 3.65321 F F 4.17e+20 1.29795e-14 1 dsx
Report srcpi bgdpi arf 3 X080400.11+650249.5 chandra ccd7 661.109 583.689 35.0014 5.9166 0.00523697 0.000885252 22.3283 1 1.55379 0.796458 0.382002 4.85829 A F 4.18e+20 4.70428e-14 1 dsx
Report srcpi bgdpi arf 4 X080417.98+650205.0 chandra ccd7 430.833 492.333 5.61008 2.4495 0.000839388 0.000366498 3.57882 0.998986 0.627733 0.492 177.373 2.99283 F F 4.17e+20 6.40031e-15 1 dx
Report srcpi bgdpi arf 5 X080430.50+645952.9 chandra ccd7 270.397 224.278 35.6224 6.69996 0.00532988 0.00100246 22.7245 1 0.420546 0.420546 0 0.572376 F F 4.18e+20 4.10293e-14 1 dsx

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