  The reanalysis of the published experimental data from reaction
Co-59(p,2gamma)Ni-60 was performed. The region of the most probable values of
level density and radiative strength functions of cascade gamma-transitions was
determined. The obtained data were rather precisely approximated by the V.M.
Strutinsky model and semi-phenomenological model - for strength functions. The
region of appearance and magnitude of maximal errors of the calculated
cross-section of nucleon emission in evaporation spectra in traditional methods
of their analysis were determined as well. There was for the first time
obtained methodically correct information on the radiation strength function of
primary gamma-transitions in diapason of neutron binding energy with averaging
over large set of initial levels.
