All Tables

Table 1: Atmospheric parameters derived from independent UV spectra.
Table 2: Periodicities identified using pre-whitening analysis for the HST FOS light curve, during the sforzando, in 1996, both for the total UV (1196-2484 Å) and zeroth-order light obtained with HST FOS. The times of maxima ( $T_{\rm max}$ ) for UV and zeroth-order data are given in relation to T₀=2 450 311.8058746 BCT.
Table 3: Probability (P) for a mode to be $\ell =1$ or 2, for the best model, with $T_{{\rm eff}}=23~900$ K and $\log g=7.91$ , in the FOS data.