_version_ 1866916302035091456
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