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Kepler Stars Observed with the LAMOST Instrument

Joanna Molenda-Żakowicz
Astronomical Institute, University of Wroclaw

I introduce the Chinese Large sky Area Multi-Object fiber Spectroscopic Telescope (LAMOST) and its application to the observations of selected stars in the Kepler field of view. I outline the method of the analysis which will be used to derive the atmospheric parameters of those stars, and I show the first results obtained for the Kepler targets observed with LAMOST in summer 2010.

2012 January 25, 13:30

Centro de AstrofÝsica da Universidade do Porto (Auditorium)
Rua das Estrelas, 4150-762 Porto

Instituto de Astrof├şsica e Ci├¬ncias do Espa├žo Universidade do Porto Faculdade de Ciências da Universidade de Lisboa Funda├ž├úo para a Ci├¬ncia e a Tecnologia
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