Abstract
We present a measurement of the ratio R = Γ(\keg;\Estar>30\mev,\qstar>20^\circ)Γ(\kegf) of data corresponding to about 3.5 million Ke3(g) events and about 9000 radiative events. Our result is R=(924 +/- 23(stat) +/-16(syst)10^{-5} for the branching ratio and X=-2.3 +/- 1.3(stat) +/- 1.4(syst) for the parameter describing direct emission.
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