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 < \mathrm { [ 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 .