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Seventy-eight high-resolution Stokes V, Q and U spectra of the B8Iaesupergiant Rigel were obtained with the ESPaDOnS spectropolarimeter at CFHT andits clone NARVAL at TBL in the context of the Magnetism in Massive Stars(MiMeS) Large Program, in order to scrutinize this core-collapse supernovaprogenitor for evidence of weak and/or complex magnetic fields. In this paperwe describe the reduction and analysis of the data, the constraints obtained onany photospheric magnetic field, and the variability of photospheric and windlines.

Searching for Weak or Complex Magnetic Fields in Polarized Spectra of Rigel