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Table 5

Inferred effective temperatures of the benchmark stars from the 3D non-LTE model (see Figs. 79 for illustrations of the 3D non-LTE fits).

ΔTeff∕K
Star Teff∕K Spectrum
Sun 5772 ± 1 KPNO 5721 ±36 5709±19 5710±33 − 51±36 − 63±19 − 62±33
Procyon 6556 ± 84 FOCES 6569 ±37 6670±52 6549±50 13±92 114±99 − 7±98
HD 103095 5140 ± 49 FOCES 5119 ±63 5002±26 4760±173 − 21±80 − 138±56 − 380±180
HD 84937 6371 ± 84 FOCES 6357 ±45 6290±38 6324±67 − 14±95 − 81± 92− 47±108
HD 140283 5787 ± 48 FOCES 5815 ±65 5793±53 5709±83 28±81 6±71 − 78±96
HD 122563 4636 ± 37 UVES 4652 ±111 4495±85 4558±165 16±117 − 141±92 − 78±169

Notes. The 1σ uncertainties in the 3D non-LTE models take into account the uncertainties in the adopted surface gravities and metallicities, and uncertainties in placing the continuum, given in Table 1, as well as the formal fitting error. The uncertainties in the continuum placement dominate, except for H α in HD 103095, where the uncertainty in dominates. The last three columns show the differences between the models and the reference values adopted from the literature (Col. 2, also Table 1), with the uncertainties combined in quadrature (see Fig. 10 for an illustration of these differences).

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