  We report results from the high resolution spectral analysis of the 107 metal
rich (mostly [Fe/H]$\ge$7.67 dex) target stars from the Calan-Hertfordshire
Extrasolar Planet Search program observed with HARPS. Using our procedure of
finding the best fit to the absorption line profiles in the observed spectra,
we measure the abundances of Na, Mg, Al, Si, Ca, Ti, Cr, Mn, Fe, Ni, Cu, and
Zn, and we then compare them with known results from different authors. Most of
our abundances agree with these works at the level of $\pm$0.05 dex or better
for the stars we have in common. However, we do find systematic differences
that make direct inferences difficult. Our analysis suggests that the selection
of line lists and atomic line data along with the adopted continuum level
influence these differences the most. At the same time, we confirm the positive
trends of abundances versus metallicity for Na, Mn, Ni, and to a lesser degree,
Al. A slight negative trend is observed for Ca, whereas Si and Cr tend to
follow iron. Our analysis allows us to determine the positively skewed normal
distribution of projected rotational velocities with a maximum peaking at 3 km
s$^{-1}$. Finally, we obtained a Gaussian distribution of microturbulent
velocities that has a maximum at 1.2 km s$^{-1}$ and a full width at half
maximum $\Delta v_{1/2}=$0.35 km s$^{-1}$, indicating that metal rich dwarfs
and subgiants in our sample have a very restricted range in microturbulent
velocity.
