Theoretical reaction rates in the temperature range 0.01 \times 10 ^ { 9 } \leq T ( { K } ) \leq 10.0 \times 10 ^ { 9 } are calculated in the statistical model ( Hauser-Feshbach formalism ) for targets with 10 \leq Z \leq 83 ( Ne to Bi ) and for a mass range reaching the neutron and proton driplines .
Reactions considered are ( n , \gamma ) , ( n , p ) , ( n , \alpha ) , ( p , \gamma ) , ( p , \alpha ) , ( \alpha , \gamma ) , and their inverse reactions .
Reaction rates as a function of temperature for thermally populated targets are given by analytic seven parameter fits .
To facilitate comparison with experimental rates , the stellar enhancement factors are also tabulated .
Two complete sets of rates have been calculated , one of which includes a phenomenological treatment of shell quenching for neutron-rich nuclei .
These extensive datasets are provided on-line as electronic files , while a selected subset from one calculation is given as printed tables .
A summary of the theoretical inputs and advice on the use of the provided tabulations is included .