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Fig. 1.
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FORS2 observations of the reference magnetic massive star HD 45166. In the left panel, the solid lines show the recorded Stokes I and Stokes V spectra and the diagnostic NV spectra, from top to bottom. In the right panel, we show the regression detection of the mean longitudinal magnetic field with ⟨Bz⟩all = −1107 ± 80 G.
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