  We have made a clear detection of excess power, providing strong evidence for
solar-like oscillations in the G2 subgiant beta Hyi. We observed this star over
five nights with the UCLES echelle spectrograph on the 3.9-m Anglo-Australian
Telescope, using an iodine absorption cell as a velocity reference. The time
series of 1196 velocity measurements shows an rms scatter of 3.30 m/s, and the
mean noise level in the amplitude spectrum at frequencies above 0.5 mHz is 0.11
m/s. We see a clear excess of power centred at 1.0 mHz, with peak amplitudes of
about 0.5 m/s, in agreement with expectations for this star. Fitting the
asymptotic relation to the power spectrum indicates the most likely value for
the large separation is 56.2 microHz, also in good agreement with the known
properties of beta Hyi.
