  Recently announced magnetic models for four SPB and {\beta} Cep stars, along
with magnetic detections for two additional stars, have potentially doubled the
number of known magnetic SPB and \beta Cep stars (see Grunhut et al., these
proceedings). We have reanalyzed the published data and re-reduced archival low
resolution spectropolarimetry collected with the FORS1/2 instruments at VLT on
which the models were based, and compare them with high resolution data from
the ESPaDOnS spectropolarimeter at CFHT, investigating previously noted
inconsistencies between results from the two instruments.
