  $K$ and evolutionary corrections are given for the E, Sa and Sc Hubble types
for the $U, B, V, R, I, J, H, K$ filters of the Johnson -- Bessell \& Brett
photometric system and the $gri$ filters of the modified Thuan \& Gunn system
up to the redshift $z=3$. Their dependence on the time scale of star formation
in ellipticals is investigated. The corrections are computed according to an
evolutionary synthesis model that reproduces the integrated galaxy spectrum in
the range 1000-25\,000 \AA; such a model makes use of an infrared observed
stellar library and its results are compared with nearby galaxies. Evolving
spectral energy distributions of the various Hubble types, as well as
optical-IR and IR-IR colour evolution and adopted filter response functions are
also given.
