Astronomy & Astrophysics manuscript no. Heiter_etal_Benchmarkstars_LE c ESO 2018 September 25, 2018 Gaia FGK benchmark stars: Effective temperatures and surface gravities U. Heiter1, P. Jofré2, B. Gustafsson1; 4, A. J. Korn1, C. Soubiran3, and F. Thévenin5 1 Institutionen för fysik och astronomi, Uppsala universitet, Box 516, 751 20 Uppsala, Sweden e-mail:
[email protected] 2 Institute of Astronomy, University of Cambridge, Madingley Rd, Cambridge, CB3 0HA, U.K. 3 Univ. Bordeaux, CNRS, LAB, UMR 5804, 33270, Floirac, France 4 Nordita, Roslagstullsbacken 23, 106 91, Stockholm, Sweden 5 Université de Nice Sophia Antipolis, CNRS (UMR7293), Observatoire de la Côte d’Azur, CS 34229, 06304, Nice Cedex 4, France Received / Accepted ABSTRACT Context. In the era of large Galactic stellar surveys, carefully calibrating and validating the data sets has become an important and integral part of the data analysis. Moreover, new generations of stellar atmosphere models and spectral line formation computations need to be subjected to benchmark tests to assess any progress in predicting stellar properties. Aims. We focus on cool stars and aim at establishing a sample of 34 Gaia FGK benchmark stars with a range of different metallicities. The goal was to determine the effective temperature and the surface gravity independently of spectroscopy and atmospheric models as far as possible. Most of the selected stars have been subjected to frequent spectroscopic investigations in the past, and almost all of them have previously been used as reference, calibration, or test objects. Methods. Fundamental determinations of Teff and log g were obtained in a systematic way from a compilation of angular diameter measurements and bolometric fluxes and from a homogeneous mass determination based on stellar evolution models.