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arxiv: 0912.0561 · v1 · submitted 2009-12-03 · 🌌 astro-ph.SR · astro-ph.IM

CARMENES: Calar Alto high-Resolution search for M dwarfs with Exo-earths with a Near-infrared Echelle Spectrograph

A. Quirrenbach , P. J. Amado , H. Mandel , J. A. Caballero , I. Ribas , A. Reiners , R. Mundt , M. Abril
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C. Afonso J. L. Bean V. J. S. Bejar S. Becerril A. Boehm C. Cardenas A. Claret J. Colome L. P. Costillo S. Dreizler M. Fernandez X. Francisco R. Garrido J. I. Gonzalez Hernandez E. W. Guenther J. Gutierrez-Soto V. Joergens A. P. Hatzes T. Henning E. Herrero M. Kurster W. Laun R. Lenzen U. Mall E. L. Martin S. Martin-Ruiz D. Montes J. C. Morales R. Morales Munoz A. Moya V. Naranjo O. Rabaza A. Ramon R. Rebolo S. Reffert F. Rodler E. Rodriguez A. Rodriguez Trinidad R.-R. Rohloff M. A. Sanchez Carrasco C. Schmidt W. Seifert J. Setiawan O. Stahl J. C. Suarez G. Wiedemann C. del Burgo D. Galadi E. Sanchez-Blanco W. Xu
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classification 🌌 astro-ph.SR astro-ph.IM
keywords altocalardwarfsnear-infraredcarmenesechelleexo-earthshigh-resolution
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CARMENES, Calar Alto high-Resolution search for M dwarfs with Exo-earths with a Near-infrared Echelle Spectrograph, is a study for a next-generation instrument for the 3.5m Calar Alto Telescope to be designed, built, integrated, and operated by a consortium of nine German and Spanish institutions. Our main objective is finding habitable exoplanets around M dwarfs, which will be achieved by radial velocity measurements on the m/s level in the near-infrared, where low-mass stars emit the bulk of their radiation.

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