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We report laboratory measurements of the Zeeman response of lines in the 0-0 Wing-Ford band of the F-X system ( λ  ~ 1 μ m) of FeH, measured in magnetic fields 0.3 – 0.5 Tesla. New Lande factors are used to deduce the magnetic field in sunspots from Stokes V profiles recorded at the solar telescope THEMIS. The magnetic field deduced from atomic lines (Ti, Fe) is slightly higher than that found from FeH.

Laboratory determination of Landé factors for the molecular radical FeH