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 X191425.95+245642.3 xmm pn 320.998 307.371 4164.9 77.5991 0.540645 0.0100731 96.6566 1 5.64974 5.64974 0 1.76701 F T 6.40067 5.96335e-13 1 dsxf
Report srcpi bgdpi arf rmf 1 X191426.05+245642.6 xmm mos2 320.708 307.446 842.203 33.4495 0.148639 0.00590346 67.9443 1 5.734 4.82751 49.7704 1.75228 F T 6.40042 1.24083e-12 1 dsxf
Report srcpi bgdpi arf 2 X191436.28+250452.8 xmm mos1 288.729 420.142 28.7862 9.09178 0.00515178 0.00162713 4.50107 0.999978 3.77826 3.77826 0 8.83603 F F 6.42783 1.36178e-13 1 dsx
Report srcpi bgdpi arf 1 X191456.37+245113.4 xmm mos1 225.851 231.807 20.8446 6.98376 0.0037305 0.00124986 3.25931 0.998734 9.20308 4.20998 225.845 7.12258 F T 6.2567 8.5568e-14 1 dsx
Report srcpi bgdpi arf 2 X191436.08+250453.1 xmm mos2 289.355 420.202 22.734 7.30503 0.00401229 0.00128925 1.83405 0.965132 5.32019 5.32019 0 8.84692 F F 6.42831 1.20553e-13 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 - 10.00 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), A = 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