All Tables

Table 1: Journal of new observations. Observatory code: ChR = Château-Renard Observatory (France), XL = Xinglong Station (China), SFO = Sulphur Flats Observatory (USA), RO = Rockville Observatory (USA), McD = McDonald Observatory (USA), MR = Mo i Rana Observatory (Norway). Notes: a) 5 nights in filter B (5 h of data and 7 times of maximum) and 4 nights in R (4 h and 4 maxima), b) no filter was used on 2 of the 5 nights, c) filter S is Schott BG40, centred at $\lambda =5000$ Å (Zhou et al. 2005), d) one night without filter and one night using Johnson V filter.
Table 2: New times of light maximum of BL Cam. $T_{\max}$ is in HJD-2 400 000. Observatory code as in Table 1. Whenever quoted B, R it means that the corresponding $T_{\max}$ was determined as the mean value.
Table 3: Amplitudes, $\Delta V_0$ and $\Delta V_1$ , of f₀=25.5769 cd^-1 and f₁, respectively, determined from different data sets by Fourier analysis.
Table 4: Summary of frequencies in the range 31-32 cd^-1. (*) Possible alias (see Note e) in Table 3).
Table 5: Results of Fourier analysis applied to the 1996 data set of Zhou et al. (1999). The sigma of the residuals is 28.6 mmag.
Table 6: Results of Fourier analysis applied to the 1999 data set of Zhou et al. (2001). The sigma of the residuals is 13.7 mmag.
Table 7: Frequencies detected close to the main pulsation f₀. Sources as in Table 3.
Table 8: Frequencies detected close to f₀. Only peaks with ${\it S/N}\geq 4.0$ are listed.
Table 9: Orbital elements of the possible BL Cam binary system.