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 X225357.48+160856.9 chandra ccd7 614.373 530.021 185.494 14.4223 0.0101582 0.00078981 7.44817 1 0.492 0.492 21.0098 0.50646 F T 6.63e+20 0 1 dpb
Report 3 X225352.82+160943.0 chandra ccd7 751.338 624.09 88.9604 9.69847 0.00487175 0.000531118 3.57204 0.999775 0.436646 0.436646 0 0.888815 F F 6.64e+20 0 1 ds
Report 5 X225358.15+160900.2 chandra ccd7 594.625 536.583 43.1503 7.54995 0.00236304 0.000413458 1.73262 0.957648 0.634805 0.492 129.39 0.585084 T F 6.63e+20 0 1 db
Report 9 X225357.75+160853.5 chandra ccd7 607.017 523.572 20304.5 146.765 1.11194 0.00803731 815.291 1 0.444852 0.41056 10.359 0.590867 F T 6.63e+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