Table 2: Oscillations extracted from the combined light curve of PG 0911+456. The uncertainty on the frequencies is estimated to be about 1/10th of the frequency resolution, i.e. around 0.02 $\mu $Hz, while the error on the amplitude is derived from the least-squares fit to the light curve. The frequencies and amplitudes detected by Koen et al. (1999) are also listed.
Rank Period Frequency Amplitude $f_{\rm Koen}$ $A_{\rm Koen}$
  (s) ($\mu $Hz) (%) ($\mu $Hz) (%)
4 192.551 5193.42 $0.082\pm0.005$    
6 168.784 5924.73 $0.054\pm0.005$    
2 165.687 6035.49 $0.223\pm0.005$ 6036.2 0.44
3 161.554 6189.89 $0.098\pm0.005$ 6190.9 0.24
5 157.581 6345.92 $0.080\pm0.005$    
1 155.767 6419.85 $0.755\pm0.005$ 6419.3 0.61
7 149.027 6710.20 $0.050\pm0.005$    


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