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Table 3

Derived A(Eu) abundances for IAG and KPNO flux and disccentre spectra.

Data 1DLTE 1D NLTE 3D LTE 3D NLTE
IAG flux 0.57 0.58 0.57 0.55
IAG µ = 1.0 0.58 0.58 0.59 0.57
KPNO flux 0.59 0.60 0.59 0.57
KPNO µ = 1 .0 0.60 0.60 0.60 0.57

Notes. The average error for all of the measurements is ~0.06 dex, where the dominant source of error is the uncertainty on the ƒ-value (based on that reported in Lawler et al. 2001).

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