Swift-UVOT U and UVW2 measurements and time-averaged optical magnitudes and fluxes measured with ATOM in R,B, and I Bessel filters.
|[eV]||[10-12 erg cm-2 s-1]||%|
Notes.The last column gives the probability obtained when fitting the time series with a constant function. Magnitudes are not corrected for Galactic extinction, whereas fluxes are dereddened using the values of Schlegel et al. (1998).
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