  We report the detection of two new planets orbiting the K giants HD 86950 and
HD 222076, based on precise radial velocities obtained with three instruments:
AAT/UCLES, FEROS, and CHIRON. HD 86950b has a period of 1270$\pm$57 days at
$a=2.72\pm$0.08 AU, and m sin $i=3.6\pm$0.7 Mjup. HD 222076b has $P=871\pm$19
days at $a=1.83\pm$0.03 AU, and m sin $i=1.56\pm$0.11 Mjup. These two giant
planets are typical of the population of planets known to orbit evolved stars.
In addition, we find a high-amplitude periodic velocity signal ($K\sim$50 m/s)
in HD 29399, and show that it is due to stellar variability rather than
Keplerian reflex motion. We also investigate the relation between planet
occurrence and host-star metallicity for the 164-star Pan-Pacific Planet Search
sample of evolved stars. In spite of the small sample of PPPS detections, we
confirm the trend of increasing planet occurrence as a function of metallicity
found by other studies of planets orbiting evolved stars.
