I will speak of new observational strategies in order to reduce as much as possible solar perturbations for GK stars (p modes, granulation, mesogranulation and supergranulation). Planets detection limits will be calculated in mass-period diagram and we will see that we can still go down in the detectable mass of planets, nearly to earth mass.
2008 November 05, 13:30
Centro de AstrofÝsica da Universidade do Porto (Auditorium)
Rua das Estrelas, 4150-762 Porto