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 X025341.12+130101.6 xmm mos1 281.485 287.038 67.8404 18.096 0.00633676 0.00169029 4.21032 0.999975 12.8482 12.8482 0 1.54223 78.306 15.8212 -0.663833 0.23545 F T 9.55e+20 6.45663e-14 1 dbsx
Report srcpi bgdpi arf 2 X025241.81+125710.2 xmm pn 480.766 233.113 -0.526296 4.84057 -0.000664356 0.00611037 -0.138087 0.514835 10.875 10.875 0 14.0416 -3.20498 1.01663 1 6.2099 F F 9.36e+20 0 1 d
Report srcpi bgdpi arf 4 X025341.19+130051.5 xmm pn 281.228 284.722 25.5961 8.09909 0.0323106 0.0102237 3.93131 0.999822 11.2381 11.2381 0 1.63749 21.3255 7.12072 -0.499355 0.322642 F T 9.55e+20 9.67437e-14 1 dsx
Report srcpi bgdpi arf 5 X025400.96+130405.2 xmm pn 214.834 329.262 15.8275 7.78525 0.0199795 0.00982753 2.43095 0.99092 7.84898 3.405 88.8604 6.49182 11.3384 2.38897 -0.651942 0.466014 F F 9.72e+20 1.18571e-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