Astronomy & Astrophysics

Table 1: List of telescopes and instruments involved in the multisite campaign.
Table 2: Properties of V351 Ori and comparison stars.
Table 4: Frequencies, amplitudes and phases derived from the Fourier analysis of the data. Phases are calculated with respect to HJD = 24 552 500.000 The uncertainty on the frequency is $\sim$ 0.03 c/d. The last column lists the signal-to-noise ratio (in amplitude) calculated as described in the text (see Sect. 3).
Table 5: Comparison between frequencies extracted from the analysis of the winter 2001 and winter 2002 campaigns and the whole dataset. The uncertainties on the frequencies for each data set are also indicated.
Table 6: Frequencies extracted in order of decreasing amplitude from the whole data set using various methods (see text). All frequencies in the table are in c/d.
Table 7: Comparison with previous works. The labels "(P)'' and "(RD)'' indicate if the frequency has been detected on the basis of photometric or radial velocities data. An uncertain correspondence of previous frequencies with the present work is marked by a question mark. The uncertainties on the frequencies are also indicated.
Table 8: Stellar parameters from the best-fit models.
Table 3: Journal of the observations.