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| Format: | Preprint |
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2024
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| Online Access: | https://arxiv.org/abs/2406.18317 |
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| _version_ | 1866916302035091456 |
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| author | Chazelas, Bruno Ivanisenko, Yevgeniy Lanotte, Audrey Diaz, Pablo Santos Genolet, Ludovic Sordet, Michael Hughes, Ian Lovis, Christophe Schmidt, Tobias M. Amate, Manuel Castro, José Peñate Moreno, Afrodisio Vega Tenegi, Fabio Simoes, Roberto Hernández, Jonay I. González Osorio, María Rosa Zapatero Piqueras, Javier Dávila, Tomás Belenguer Ortega, Rocío Calvo González, Roberto Varas Fernández, Luis Miguel González Amado, Pedro J. Kern, Jonathan Dionies, Frank Bauer, Svend-Marian Önel, Hakan Järvinen, Arto Brynnel, Joar Füßlein, Christine Bellido, Olga Weingrill, Jörg Giannone, Domenico Gaessler, Wolfgang lehmitz, Michael Kaminski, Adrian Stilz, Ingo Sigwarth, Michael Marconi, Alessandro Di Marcantonio, Paolo Oliva, Ernesto Coretti, Igor Aliverti, Matteo Pariani, Giorgio Cabona, Lorenzo Radaelli, Edouardo Maria Alberto Scalera, Marcello Balestera, Andrea |
| author_facet | Chazelas, Bruno Ivanisenko, Yevgeniy Lanotte, Audrey Diaz, Pablo Santos Genolet, Ludovic Sordet, Michael Hughes, Ian Lovis, Christophe Schmidt, Tobias M. Amate, Manuel Castro, José Peñate Moreno, Afrodisio Vega Tenegi, Fabio Simoes, Roberto Hernández, Jonay I. González Osorio, María Rosa Zapatero Piqueras, Javier Dávila, Tomás Belenguer Ortega, Rocío Calvo González, Roberto Varas Fernández, Luis Miguel González Amado, Pedro J. Kern, Jonathan Dionies, Frank Bauer, Svend-Marian Önel, Hakan Järvinen, Arto Brynnel, Joar Füßlein, Christine Bellido, Olga Weingrill, Jörg Giannone, Domenico Gaessler, Wolfgang lehmitz, Michael Kaminski, Adrian Stilz, Ingo Sigwarth, Michael Marconi, Alessandro Di Marcantonio, Paolo Oliva, Ernesto Coretti, Igor Aliverti, Matteo Pariani, Giorgio Cabona, Lorenzo Radaelli, Edouardo Maria Alberto Scalera, Marcello Balestera, Andrea |
| contents | We present here the preliminary design of the RIZ module, one of the visible spectrographs of the ANDES instrument 1. It is a fiber-fed high-resolution, high-stability spectrograph. Its design follows the guidelines of successful predecessors such as HARPS and ESPRESSO. In this paper we present the status of the spectrograph at the preliminary design stage. The spectrograph will be a warm, vacuum-operated, thermally controlled and fiber-fed echelle spectrograph. Following the phase A design, the huge etendue of the telescope will be reformed in the instrument with a long slit made of smaller fibers. We discuss the system design of the spectrographs system. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_18317 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | ANDES, the high-resolution spectrograph for the ELT: RIZ Spectrograph preliminary design Chazelas, Bruno Ivanisenko, Yevgeniy Lanotte, Audrey Diaz, Pablo Santos Genolet, Ludovic Sordet, Michael Hughes, Ian Lovis, Christophe Schmidt, Tobias M. Amate, Manuel Castro, José Peñate Moreno, Afrodisio Vega Tenegi, Fabio Simoes, Roberto Hernández, Jonay I. González Osorio, María Rosa Zapatero Piqueras, Javier Dávila, Tomás Belenguer Ortega, Rocío Calvo González, Roberto Varas Fernández, Luis Miguel González Amado, Pedro J. Kern, Jonathan Dionies, Frank Bauer, Svend-Marian Önel, Hakan Järvinen, Arto Brynnel, Joar Füßlein, Christine Bellido, Olga Weingrill, Jörg Giannone, Domenico Gaessler, Wolfgang lehmitz, Michael Kaminski, Adrian Stilz, Ingo Sigwarth, Michael Marconi, Alessandro Di Marcantonio, Paolo Oliva, Ernesto Coretti, Igor Aliverti, Matteo Pariani, Giorgio Cabona, Lorenzo Radaelli, Edouardo Maria Alberto Scalera, Marcello Balestera, Andrea Instrumentation and Methods for Astrophysics We present here the preliminary design of the RIZ module, one of the visible spectrographs of the ANDES instrument 1. It is a fiber-fed high-resolution, high-stability spectrograph. Its design follows the guidelines of successful predecessors such as HARPS and ESPRESSO. In this paper we present the status of the spectrograph at the preliminary design stage. The spectrograph will be a warm, vacuum-operated, thermally controlled and fiber-fed echelle spectrograph. Following the phase A design, the huge etendue of the telescope will be reformed in the instrument with a long slit made of smaller fibers. We discuss the system design of the spectrographs system. |
| title | ANDES, the high-resolution spectrograph for the ELT: RIZ Spectrograph preliminary design |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2406.18317 |