Table 1: Journal of observations: begin and end of the run, the number of observations n, the mean values $\langle m\rangle$ and rms deviations of the mean $\sigma _m$ and the filter.
$t_{\rm start},$ 24..... $t_{\rm end},$ 24..... n $\hfill\langle m\rangle$ $\sigma _m$ Filter
52 635.2721 52 635.3388   95 15.052 0.147 V
52 638.2627 52 638.3379  177 14.941 0.137 V
53 035.0390 53 035.1655  217 15.042 0.176 V
53 036.1058 53 036.2677  278 14.953 0.163 V
53 052.9374 53 053.1193  299 15.023 0.171 V
53 383.0829 53 383.1145   18 15.046 0.147 V
53 383.0838 53 383.1153   17  2.800 0.149 R
53 384.1352 53 384.1648   14 14.914 0.173 V
53 384.1365 53 384.1657   14  2.678 0.171 R
53 385.9945 53 386.1484   66 15.049 0.193 V
53 385.9955 53 386.1494   69  2.811 0.184 R
53 404.9714 53 405.1264   72 15.077 0.206 V
53 404.9726 53 405.1250   70  2.848 0.197 R
52 635.2721 53 405.1264 1236 15.005 0.173 all V
53 383.0838 53 405.1250  170  2.814 0.189 all R


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Observations and comparison stars
3 Separation of spin and orbital variability
4 Color variability with the phase of orbital and spin period
5 194-minute orbital period
6 Variability of the spin period
7 Conclusions
References
List of tables
List of figures