  Several of the many proposed Dark Matter candidate particles, already
investigated with lower exposure and a higher software energy threshold, are
further analyzed including the first DAMA/LIBRA--phase2 data release, with an
exposure of 1.13 ton $\times$ yr and a lower software energy threshold (1 keV).
The cumulative exposure above 2 keV considering also DAMA/NaI and
DAMA/LIBRA--phase1 results is now 2.46 ton $\times$ yr. The analysis permits to
constraint the parameters' space of the considered candidates restricting their
values -- with respect to previous analyses -- thanks to the increase of the
exposure and to the lower energy threshold.
