All Tables

Table 1: Journal of the observations. Note that the data coming from Sierra Nevada and San Pedro Martir (SPM) have been transformed in the Johnson system as discussed in Sect. 2.2.
Table 2: List of telescopes and instruments involved in the multisite campaign. SCP means Single Channel Photometer; TCP means Three Channel Photometer. To give an idea of the relative photometric precision of each site, the last column shows the white noise in the Fourier space (amplitude) for each site. All the calculations are in the V filter except for Loiano (2002) and SARA sites for which we have only B filter data.
Table 3: $uvby{\beta }$ indices obtained for IP Per and comparison stars. The pairs below the star names are the number of points collected for each object in uvby and $\beta$ , respectively. The numbers below the measures show the errors (in mmag). The values given by Olsen (1996, private communication) are listed in the bottom part.
Table 4: Frequencies, amplitudes and confidence levels for the three datasets analysed in this paper. The error bars on the frequencies are $\pm$ 0.11 c/d, $\pm$ 0.15 c/d and $\pm$ 0.25 c/d for the datasets 2003 V, 2003 B and 2002 B datasets, respectively. Note that for the 2003 Band 2002 B datasets the frequencies are not listed by decreasing amplitude, but by correspondence with the 2003 V dataset frequencies (see text).