A&A 600, A69 (2017) Astronomy DOI: 10.1051/0004-6361/201629967 & c ESO 2017 Astrophysics SWEET-Cat update and FASMA A new minimization procedure for stellar parameters using high-quality spectra?,?? D. T. Andreasen1; 2, S. G. Sousa1, M. Tsantaki3, G. D. C. Teixeira1; 2, A. Mortier4, N. C. Santos1; 2, L. Suárez-Andrés5; 6, E. Delgado-Mena1, and A. C. S. Ferreira1; 2 1 Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762 Porto, Portugal e-mail:
[email protected] 2 Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, Rua Campo Alegre, 4169-007 Porto, Portugal 3 Instituto de Radioastronomía y Astrofísica, IRyA, UNAM, Campus Morelia, A.P. 3-72, 58089 Michoacán, Mexico 4 Centre for Exoplanet Science, SUPA, School of Physics and Astronomy, University of St Andrews, St Andrews KY16 9SS, UKSUPA, School of Physics and Astronomy, University of St Andrews, St Andrews KY16 9SS, UK 5 Depto. Astrofísica, Universidad de La Laguna (ULL), 38206 La Laguna, Tenerife, Spain 6 Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain Received 27 October 2016 / Accepted 17 January 2017 ABSTRACT Context. Thanks to the importance that the star-planet relation has to our understanding of the planet formation process, the precise determination of stellar parameters for the ever increasing number of discovered extrasolar planets is of great relevance. Furthermore, precise stellar parameters are needed to fully characterize the planet properties. It is thus important to continue the efforts to determine, in the most uniform way possible, the parameters for stars with planets as new discoveries are announced.