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B fields in OB stars (BOB): low-resolution FORS2 spectropolarimetry of the first sample of 50 massive stars

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Figure

Table 1. Comparison between the reduction and analysis procedures applied within the two adopted pipelines
Fig. 1. Overview of the results of the analysis of the FORS2 data of HD 46328, collected on 7 April 2013, considering the hydrogen lines, using the Bonn pipeline
Fig. 2. Overview of the results of the analysis of the FORS2 data of HD 46328, collected on 9 April 2013, considering the hydrogen lines, using the Potsdam pipeline
Figure 4 shows the phase plot obtained using the FORS1 and FORS2 measurements, and the results of the magnetic field modelling given by Hubrig et al
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