Handler G. (1,2), Xcov3,Xcov7,Xcov12,Xcov20,Xcov21,Xcov22 teams
(1) Institut für Astronomie, Universität Wien, Türkenschanzstraße 17, A-1180 Wien, Austria
(2) South african Astronomical Observatory, P.O. box 9, Observatory 7935, South Africa
In: The 6th W.E.T. Workshop, ed. J.E. Solheim and E. Meistas, Baltic Astronomy 12, 11
Abstract. I have collected all the WET archival data on the pulsating DB white dwarf stars (DBVs) and re-reduced them. In addition, the WET has recently observed three DBVs. Preliminary results on PG1115+158, PG1351+489, KUV05134+2605, PG1654+160 and PG1456+103 are presented, and the future of the data is outlined.Key words: stars: white dwarfs, oszillations, individual: PG1115+158, PG1351+489, KUV05134+2605, PG1654+160, PG1456+103
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