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, 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

TL;DR
CARMENES is a planned high-resolution near-infrared spectrograph for the Calar Alto Telescope aimed at detecting habitable exoplanets around M dwarfs through precise radial velocity measurements.
Contribution
This paper introduces the design and objectives of CARMENES, a new instrument dedicated to exoplanet discovery around M dwarfs using near-infrared spectroscopy.
Findings
Design of a next-generation spectrograph for M dwarf observations
Expected to achieve m/s radial velocity precision
Aims to identify habitable exoplanets
Abstract
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
