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 X024031.49+611344.7 xmm pn 318.82 311.039 3105.03 70.1133 0.806752 0.0182169 72.9669 1 5.83677 5.50923 21.8514 1.74626 F T 1.08584 4.34687e-12 1 dsxf
Report srcpi bgdpi arf 1 X024031.41+611341.8 xmm mos2 318.948 310.381 37.8646 8.47119 0.44149 0.0987715 6.96837 1 5.12318 5.12318 0 1.71864 F T 1.08495 6.26691e-12 1 dsx
Report srcpi bgdpi arf rmf 1 X024031.42+611344.4 xmm mos1 318.926 310.968 595.456 29.0031 0.393503 0.0191665 46.5935 1 5.02225 5.02225 0 1.75433 F T 1.08557 6.48197e-12 1 dsxf
Report srcpi bgdpi arf 2 X024002.26+610741.5 xmm mos2 367.558 227.635 11.3604 6.04283 0.132459 0.0704576 2.0907 0.973795 3.5495 0.761007 115.622 7.16331 A F 0.969999 2.05013e-11 1 dsx
Report srcpi bgdpi arf 3 X024002.15+610743.3 xmm mos1 367.73 227.799 337.416 24.4003 0.417507 0.0301921 26.4022 1 10.875 10.875 0 7.17392 F T 0.970107 1.29736e-11 1 dx

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