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We present our ongoing survey of ~1000 GK-giants with the 9.2-m Hobby-EberlyTelescope in search for planets around evolved stars. The stars selected forthis survey are brighter than 11 mag and are located in the section of theHR-diagram, which is approximately delimited by the main sequence, theinstability strip, and the coronal dividing line. We use the High ResolutionSpectrograph to obtain stellar spectra for radial velocity measurements with a4-6 m/s precision. So far, the survey has discovered a planetary-mass companionto the K0-giant HD 17092, and it has produced a number of plausible planetcandidates around other stars. Together with other similar efforts, our programprovides information on planet formation around intermediate mass mainsequence-progenitors and it will create the experimental basis with which tostudy dynamics of planetary systems around evolving stars.

A HET search for planets around evolved stars