  The quasielastic charged current (CCQE) $\nu_e n \rightarrow e^- p$
scattering is the dominant mechanism to detect appearance of a $\nu_e$ in an
almost $\nu_\mu$ flux at the 1 GeV scale. Actual experiments show a precision
below 1% and between less known background contributions, but necessary to
constraint the event excess, we have the radiative corrections. A consistent
model recently developed for the simultaneous description of elastic and
radiative $\pi N$ scattering, pion-photoproduction and single pion production
processes, both for charged and neutral current neutrino-nucleon scattering, is
extended for the evaluation of the radiative $\nu_l N\rightarrow \nu_l N
\gamma$ cross section. Our results are similar to a previous (but inconsistent)
theoretical evaluation in the low energy region, and show an increment in the
upper region where the $\Delta$ resonance becomes relevant.
