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 X191437.54+502854.9 chandra ccd7 213.945 239.846 613.381 25.1052 0.303333 0.0124152 149.254 1 0.422843 0.380888 333.578 0.425918 F F 6.16e+20 3.05342e-12 1 dsxf
Report 1 X191348.83+502810.4 chandra ccd3 16.8335 462.333 5.78439 2.4495 0.00286064 0.00121139 12.4127 1 0.492 0.492 122.886 8.19 F F 6.08e+20 0 1 d
Report 2 X191450.08+502714.1 chandra ccd6 489.167 933.5 2.95185 1.73205 0.00145979 0.000856561 6.65933 0.999947 0.510281 0.492 28.155 2.23427 F F 6.18e+20 0 1 d
Report 1 X191451.39+502557.3 chandra ccd6 463.5 777.5 1.9686 1.41421 0.000973541 0.000699378 4.44114 0.998908 0.492 0.492 90 3.37293 F F 6.18e+20 0 1 d

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