  We present results from high-resolution (R $\sim 40,000$) spectroscopic
observations of over 200 metal-poor stars, mostly selected from the RAVE
survey, using the Southern African Large Telescope. We were able to derive
stellar parameters for a total of 108 stars; an additional sample of 50 stars
from this same effort was previously reported on by Rasmussen et al.. Among our
newly reported observations, we identify 84 very metal-poor (VMP; [Fe/H] $<
-2.0$, 53 newly identified) stars and 3 extremely metal-poor (EMP; [Fe/H] $<
-3.0$, 1 newly identified) stars. The elemental abundances were measured for
carbon, as well as several other $\alpha$-elements (Mg, Ca, Sc, Ti), iron-peak
elements (Mn, Co, Ni, Zn), and neutron-capture elements (Sr, Ba, Eu). Based on
these measurements, the stars are classified by their carbon and
neutron-capture abundances into carbon-enhanced metal-poor (CEMP; [C/Fe] $>
+0.70$), CEMP sub-classes, and by the level of their $r$-process abundances. A
total of 17 are classified as CEMP stars. There are 11 CEMP-$r$ stars (8 newly
identified), 1 CEMP-$s$ star (newly identified), 2 possible CEMP-$i$ stars (1
newly identified), and 3 CEMP-no stars (all newly identified) in this work. We
found 11 stars (8 newly identified) that are strongly enhanced in $r$-process
elements ($r$-II; [Eu/Fe] $> +0.70$), 38 stars (31 newly identified) that are
moderately enhanced in $r$-process elements ($r$-I; $+0.30 < $ [Eu/Fe] $\leq
+0.70$), and 1 newly identified limited-$r$ star.
