All Tables

Table 1: Photometry obtained for PG 0911+456 (2006-2007).
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.
Table 3: Mode identification inferred from Model 1 and Model 2.
Table 4: Period fit for the optimal model. We list the mode identification of the observed periods together with the theoretical periods, the stability coefficient $\sigma _I$ , the kinetic energy $\log{E}$ and the rotation coefficient C_kl. Also indicated are the relative dispersion of the period fit and the amplitude rank of the observed periodicity.
Table 5: Structural parameters of PG 0911+456.