  We present a large set of theoretical isochrones, whose distinctive features
mostly reside on the greatly improved treatment of the thermally pulsing
asymptotic giant branch (TP-AGB) phase. Essentially, we have coupled the TP-AGB
tracks described in Paper I, at their stages of pre-flash quiescent H-shell
burning, with the evolutionary tracks for the previous evolutionary phases from
Girardi et al. (2000). Theoretical isochrones for any intermediate value of age
and metallicity are then derived by interpolation in the grids. We take care
that the isochrones keep, to a good level of detail, the several peculiarities
present in these TP-AGB tracks. Theoretical isochrones are then converted to
about 20 different photometric systems -- including traditional ground-based
systems, and those of recent major wide-field surveys such as SDSS, OGLE,
DENIS, 2MASS, UKIDSS, etc., -- by means of synthetic photometry applied to an
updated library of stellar spectra, suitably extended to include C-type stars.
Finally, we correct the predicted photometry by the effect of circumstellar
dust during the mass-losing stages of the AGB evolution, which allows us to
improve the results for the optical-to-infrared systems, and to simulate mid-
and far-IR systems such as those of Spitzer and AKARI. Access to the data is
provided both via a web repository of static tables
(http://stev.oapd.inaf.it/dustyAGB07 and CDS), and via an interactive web
interface (http://stev.oapd.inaf.it/cmd) that provides tables for any
intermediate value of age and metallicity, for several photometric systems, and
for different choices of dust properties.
