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We present results of our projected rotational velocities (Vsin(i))measurements of F, G and K giants obtained from the cross-correlation function(CCF) constructed from high signal to noise spectra. We also present thecalibration of the HET/HRS cross-correlation function to determine accurateprojected rotational velocities Vsin(i) for slowly-rotating F-K giants.

The PSU/TCfA Search for Planets Around Evolved Stars: Vsin(i) Measurements for Slow Rotating F-K Giants