  We present basic stellar parameters of 99 late-type G giants based on high
resolution spectra obtained by the High Dispersion Spectrograph attached to
Subaru Telescope. These stars are targets of a Doppler survey program searching
for extra-solar planets among evolved stars, with a metallicity of
-0.8<[Fe/H]<+0.2. We also derived their abundances of 15 chemical elements,
including four $\alpha$-elements (Mg, Si, Ca, Ti), three odd-Z light elements
(Al, K, Sc), four iron peak elements (V, Cr, Fe, Ni), and four neutron-capture
elements (Y, Ba, La, Eu). Kinematic properties reveal that most of the program
stars belong to the thin disk.
