Equivalent widths from GETJOB are not completely independent of the
user; differences usually arise from decisions regarding continuum regions
to be used, and over-riding the automated line fits.  All abundances in
this paper are based on EW measurements from TSH.  We investigated the
EW uncertainties by comparison with three stars measured by AMcW; also
using GETJOB.  We found typical 1$\sigma$ random errors of 3--3.5 m\AA ,
with systematic uncertainties of the same magnitude.  The AMcW EWs did lead
to slightly different atmosphere parameters and abundances: The largest 
changes were for I-245 with a 100K lower T$_{\rm eff}$ and microturbulent
velocity lower by 0.2 Km/s.  The derived [Fe/H] values were all within
0.05 dex of the values found from TSH EWs, while abundance ratios 
changed by less than 0.05 dex.