of 5.9 mÅ, indicating excellent agreement between the two studies. Below we include some notes on three of the most interesting or uncertain abundances.

Palladium
---------

A rarely measured element is the intermediate-mass neutron-capture element Pd. With A$\sim$130, it lies between the better-studied regions near Sr (A$\sim$90) and Ba (A$\sim$160). When this region was first explored in metal-poor r-process-rich stars, unexpected deviations from [$r_{ss}$]{}were found (Sneden [et al.]{} 2000 ; Johnson & Bolte 2002b). Of all the elements in this mass region, we could measure one line of Pd. Our synthesis is shown in Figure 1.

![Spectral synthesis of (left) and (right) in CS 31062-050. The solid squares are the data. The solid lines represent, in order of increasing strength and relative to our adopted log $\epsilon = -\infty$, $-0.3$ dex, 0.0 dex, and $+0.3$ dex. Several lines in these regions of the spectrum have uncertain [$gf$-values]{} and we have increased the [$gf$-value]{} for on the left and on the right above that in KUR95 to fit the spectrum.](f1.eps){width="3.0in"}

The [$gf$-value]{} is from Biémont [et al.]{} (1982) and the line list is from Johnson & Bolte (2002b). Unfortunately, none of the odd elements in this mass region, such as Ag, 