CARMENES: Calar Alto high-resolution search for M dwarfs with exo-earths with a near-infrared Echelle spectrograph
2010; SPIE; Linguagem: Inglês
10.1117/12.857777
ISSN1996-756X
AutoresA. Quirrenbach, P. J. Amado, H. Mandel, J. A. Caballero, R. Mundt, I. Ribas, A. Reiners, Miguel Abril, J. Aceituno, C. Afonso, D. Barrado, Jacob L. Bean, V. J. S. Béjar, S. Becerril, A. Böhm, M. Vázquez, A. Claret, J. Colomé, Luis P. Costillo, S. Dreizler, M. Fernández, Xavier Francisco, D. Galadí-Enríquez, R. Garrido, J. I. Gónzalez Hernández, J. Guàrdia, E. W. Guenther, J. Gutiérrez‐Soto, V. Joergens, A. P. Hatzes, J. Helmling, Thomas Henning, E. Herrero, M. Kürster, W. Laun, R. Lenzen, U. Mall, E. L. Martı́n, S. Martín‐Ruiz, E. Mirabet, D. Montes, J. C. Morales, R. Morales, A. Moya, V. Naranjo, O. Rabaza, A. Ramón, R. Rébolo, S. Reffert, F. Rodler, E. Rodrı́guez, A. Rodríguez Trinidad, R.-R. Rohloff, M. Á. Sánchez Carrasco, C. Schmidt, W. Seifert, J. Setiawan, E. Solano, O. Stahl, Clemens Storz, J. C. Suárez, U. Thiele, Karl Wagner, G. Wiedemann, M. R. Zapatero Osorio, C. del Burgo, E. Sánchez-Blanco, Wei Xu,
Tópico(s)Astronomical Observations and Instrumentation
ResumoCARMENES (Calar Alto high-Resolution search for M dwarfs with Exo-earths with Near-infrared and optical Echelle Spectrographs) is a next-generation instrument to be built for the 3.5m telescope at the Calar Alto Observatory by a consortium of Spanish and German institutions. Conducting a five-year exoplanet survey targeting ~ 300 M stars with the completed instrument is an integral part of the project. The CARMENES instrument consists of two separate spectrographs covering the wavelength range from 0.52 to 1.7 μm at a spectral resolution of R = 85, 000, fed by fibers from the Cassegrain focus of the telescope. The spectrographs are housed in a temperature-stabilized environment in vacuum tanks, to enable a 1m/s radial velocity precision employing a simultaneous ThAr calibration.
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