Spectroscopic parameters for solar-type stars with moderate-to-high rotation. New parameters for ten planet hosts
Context. Planetary studies demand precise and accurate stellar parameters as input for inferring the planetary properties. Different methods often provide different results that could lead to biases in the planetary parameters. Aims: In this work, we present a refinement of the spectral synthesis technique designed to treat fast rotating stars
Tsantaki, M. et al.
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10
2014