  Sun-like oscillations, that is p-modes excited stochastically by convective
noise, have now been observed in a number of Red Giant stars. Compared to those
seen in the Sun, these modes are of large amplitude and long period, making the
oscillations attractive prospects for observation. However, the low Q-factor of
these modes, and issues relating to the rising background at low frequencies,
present some interesting challenges for identifying modes and determining the
related asteroseismic parameters.
  We report on the analysis procedure adopted for peak-bagging by our group at
Birmingham, and the techniques used to robustly ensure these are not a product
of noise. I also show results from a number of giants extracted from multi-year
observations with the SMEI instrument.
