2896 20160701171712.0 10.1017/S1743921309030804 DOI ASTROimport-1053 Hubrig, S. 2009 New magnetic field measurements of ß Cephei stars and slowly pulsating B stars We present the results of the continuation of our magnetic survey with FORS 1 at the VLT of a sample of B-type stars consisting of confirmed or candidate ß Cephei stars and Slowly Pulsating B stars. Roughly one third of the studied ß Cephei stars have detected magnetic fields. The fraction of magnetic Slowly Pulsating B and candidate Slowly Pulsating B stars is found to be higher, up to 50%. We find that the domains of magnetic and non-magnetic pulsating stars in the H-R diagram largely overlap, and no clear picture emerges as to the possible evolution of the magnetic field across the main sequence. Briquet, M. De Cat, P. Schöller, M. Morel, T. Ilyin, I. Cosmic Magnetic Fields: From Planets, to Stars and Galaxies 259 2009 389-390 http://esoads.eso.org/abs/2009IAUS..259..389H published in NONREF