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CARMENES: Calar Alto high-Resolution search for M dwarfs with Exo-earths with Near-infrared and optical Echelle Spectrographs

Published online by Cambridge University Press:  10 November 2011

Andreas Quirrenbach
Affiliation:
Landessternwarte Königstuhl, Heidelberg, Germany email: [email protected]
Pedro J. Amado
Affiliation:
Instituto de Astrofísica de Andalucía, Granada, Spain
José A. Caballero
Affiliation:
Centro de Astrobiología, Madrid, Spain
Holger Mandel
Affiliation:
Landessternwarte Königstuhl, Heidelberg, Germany email: [email protected]
Reinhard Mundt
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg, Germany
Ansgar Reiners
Affiliation:
Insitut für Astrophysik, Göttingen, Germany
Ignasi Ribas
Affiliation:
Institut de Ciències de l'Espai, Barcelona, Spain
Miguel A. Sánchez Carrasco
Affiliation:
Instituto de Astrofísica de Andalucía, Granada, Spain
Walter Seifert
Affiliation:
Landessternwarte Königstuhl, Heidelberg, Germany email: [email protected]
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Abstract

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CARMENES (Calar Alto high-Resolution search for M dwarfs with Exo-earths with Near-infrared and optical Echelle Spectrographs) is a next-generation instrument for the 3.5 m telescope at the Calar Alto Observatory. CARMENES will conduct a five-year exoplanet survey targeting ~300 M stars. The CARMENES instrument consists of two separate fiber-fed spectrographs covering the wavelength range from 0.52 to 1.7 μm at a spectral resolution of R = 85,000. The spectrographs are housed in a temperature-stabilized environment in vacuum tanks, to enable a 1 m/s radial velocity precision employing a simultaneous emission-line calibration.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Quirrenbach, A., et al. 2010, in: Ground-based and airborne instrumentation for astronomy III, Eds. McLean, I.S., Ramsay, S.K., & Takami, H., Proc. SPIE, 7735, 1Google Scholar
Reiners, A., et al. 2010, ApJ, 710, 432CrossRefGoogle Scholar