Fig. 2

The observations of Abell 36 were obtained with FORS1 on June 3, 2005. The top panel shows the observed flux F (black solid line, in arbitrary units, and uncorrected for the instrumental response), the PV = V / I profile (red solid line centred on about 0), and the null profile NV (blue solid line, offset by −0.75% for display purposes). The null profile is expected to be centred on about zero and scattered according to a Gaussian of width σ given by the PV error bars, which are represented by light blue bars centred on about −0.75%. The slope of the interpolating lines in the bottom panels gives the mean longitudinal field from both PV (left bottom panel) and the null profile (right bottom panel) both calculated using the H Balmer and metal lines. The corresponding ⟨ Bz ⟩ and ⟨ Nz ⟩ values are −33 ± 158 G and −420 ± 161 G, respectively.
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