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We have used Lomb-Scargle periodogram analysis and Monte Carlo significancetests to detect periodicities above the 3-sigma level in the Beta Cephei starsV400 Car, V401 Car, V403 Car and V405 Car. These methods produce six previouslyunreported periodicities in the expected frequency range of excited pulsations:one in V400 Car, three in V401 Car, one in V403 Car and one in V405 Car. One ofthese six frequencies is significant above the 4-sigma level. We providestatistical significances for all of the periodicities found in these fourstars.

Application of Monte Carlo-based statistical significance determinations to the Beta Cephei stars V400 Car, V401 Car, V403 Car and V405 Car