All Tables

Table 1: Journal of observations. For each run we give the mean HJD 2 452 100+, the orbital phase coverage, and the number of obtained spectra.
Table 2: Spectral lines having their origin mainly in the primary and spectral lines with the strongest contributions of the secondary (wavelength in Å, ions, and RMT number of transition).
Table 4: Orbital solutions of RZ Cas assuming a circular orbit (solution I) as well as a non-circular orbit (solution II). The orbital period is fixed to P=1.1952572. $T_{\rm P}$ is the epoch of periastron passage, T₁ corresponds to Min I, epochs are given as HJD 2 452 100+. For comparison we list also the elements obtained by Duerbeck & Hänel (1978) from metal lines.
Table 5: Masses of the components derived from orbital solution I.
Table 6: Short-term frequencies found by successive pre-whitening. We list frequency, period, and semi-amplitude as well as the peak height S in the periodograms. Errors are given in parentheses in units of the last digit.
Table 7: High-frequency peaks found within single nights. For every run we give JD as 2 452 100+, mean orbital phase $\phi$ , frequencies in c d^-1 and corresponding amplitudes in m s^-1. f₁ and f₂ mean frequencies found very near to the frequencies f₁ and f₂ obtained from the entire data set, additional frequencies found in the high-frequency domain are listed as f_a. Errors are given in parenthesis in units of the last digit.