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Fig. 1

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The polarised spectrum of HD 94660 observed on 2007-03-22 with grism 600B. The top panel shows the normalised derivative of the observed flux, and the panel immediately below shows the observed flux F (black solid line, in arbitrary units, and not corrected for the instrument response), the PV profile (red solid line centred about 0), and the null profile (blue solid line, offset by –0.75% for display purpose). The null profile is expected to be centred about zero and scattered according to a Gaussian with σ given by the PV error bars. The PV error bars are represented with light blue bars centred about –0.75%. The slope of the interpolating lines in the bottom panels gives the mean longitudinal field from PV (left bottom panel) and from the null profile (right bottom panel) both calculated using the H Balmer lines only. The corresponding  ⟨ Bz ⟩  and  ⟨ Nz ⟩  values are  − 1885 ± 90 G and  − 192 ± 62 G, respectively.

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