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Fig. A.9

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Prewhitening steps in our frequency analysis of the β Cephei star SBL486 are shown, as well as sample light curves with the multi-periodic fit. No mode identification could be performed because of unreliable data in U. Three frequencies were included in our analysis which take the values f1 = 11.3791d-1, f2 = 13.8258d-1, f3 = 18.058d-1. The errors range from σf1 = 0.0007d-1 to σf3 = 0.001d-1. All notations and markings are the same as in Fig. A.3.

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