Table 1: Averaged observed amplitude ratios and phase differences from 2000/1 to 2004/5. Only frequencies detected in both photometric and spectroscopic data are listed. In the last two columns the predicted spherical degree from our mode identification (see Sect. 3.4) and the azimuthal number m from Zima et al. (2007) are given. For f9 no reliable results could be derived due to the influence of the close and more dominant frequency f6.
  Frequency Av/Ay $\phi_v$-$\phi_y$ $\ell $ m
  [cd-1] [mmag] [$^\circ$]    
f1 6.8980 1.44 $\pm$ 0.01 +2.96 $\pm$ 0.22 0 0
f2 7.0060 1.43 $\pm$ 0.01 -1.83 $\pm$ 0.39 1 1
f3 9.1175 1.46 $\pm$ 0.02 -1.85 $\pm$ 0.29 1 1
f4 11.5196 1.42 $\pm$ 0.01 -1.75 $\pm$ 0.50 1 0
f5 8.9606 1.45 $\pm$ 0.03 +2.35 $\pm$ 0.36 0 0
f6 9.5613 1.46 $\pm$ 0.02 -1.40 $\pm$ 0.32 1  
f7 7.3034 1.45 $\pm$ 0.06 -6.75 $\pm$ 1.61 2 0
f8 6.7953 1.38 $\pm$ 0.08 -7.26 $\pm$ 4.57 2 0
f9 9.5801 - -    
f10 6.3391 1.40 $\pm$ 0.10 -4.97 $\pm$ 5.69 2  
f11 8.6393 1.35 $\pm$ 0.09 -7.44 $\pm$ 1.58   0
f12 11.2919 1.32 $\pm$ 0.19 -3.21 $\pm$ 5.35    


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