  Following Paper I, we provide extended tables of bolometric corrections,
extinction coefficients, stellar isochrones, and integrated magnitudes and
colours of single-burst stellar populations, for the Sloan Digital Sky Survey
(SDSS) ugriz photometric system. They are tested on comparisons with DR1 data
for a few stellar systems, namely the Palomar 5 and NGC 2419 globular clusters
and the Draco dSph galaxy.
