GRASIL, a code mostly developed by
and Gian Luigi Granato to compute the spectral evolution of stellar systems taking
into account the effects of dust (win95/98/NT PCs, Linux PCs and Alpha-Digital UNIX executables are available). Of
course it may be used as well to do 'standard' no-dust spectral synthesis.
The original paper is
Silva et al 1998.
While the main features were all already present, several improvements have
been made over the years, mostly exploiting new observations (ISO, Spitzer...).