Towards stellar effective temperatures and diameters at 1 per cent accuracy for future surveys

L. Casagrande*, L. Portinari, I. S. Glass, D. Laney, V. Silva Aguirre, J. Datson, J. Andersen, B. Nordström, J. Holmberg, C. Flynn, M. Asplund

*Corresponding author for this work

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