ANDES, the high resolution spectrograph for the ELT: calibration unit(s)

The instrumentation plan for the ELT foresees the ArmazoNes high Dispersion Echelle Spectrograph (ANDES). The ANDES-project and consortium entered phase B in January 2022 and underwent several (internal and external) revisions by now to ensure that the requirements and eventually the challenging goals can be met by the physical design of the spectrograph. <br/> <br clear="all"/> Among its main scientific goals are the detection of atmospheres of exoplanets and the determination of fundamental physical constants. For this, high radial velocity precision and accuracy are required. Even though the ANDES-spectrograph is designed for maximum intrinsic stability, a calibration and thus a calibration unit is mandatory. To allow for maximum flexibility and modularity the calibration unit is physically split into three calibration units. <br/> <br clear="all"/> We show the design of the calibration units and their individual components, where possible. This includes the electronics, the mechanics, the software supporting and controlling the light guiding and calibration sources.

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Publication Details

Published
2024-08-26
DOI
https://doi.org/10.1117/12.3018745
Citations
3
Primary Topic
Astronomy and Astrophysical Research
Type
article
Field-Weighted Citation Impact
1.52

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article

ANDES, the high resolution spectrograph for the ELT: calibration unit(s)

A. Reiners, Claude LeMen, P. Huke, C. Mordasini et al.
3 citations
Astronomy and Astrophysical Research
1.52
article

ANDES, the high resolution spectrograph for the ELT: calibration unit(s)

A. Reiners, Claude LeMen, P. Huke, C. Mordasini, Richard A. McCracken, E. Giro, J. Knoche, Wolfgang Gäessler, Piotr Masłowski, P. Di Marcantonio, Driss Kouach, Jennifer Zimara, C. Broeg, F. Olchewski, Alessio Zanutta, J. Liske, Sebastian Schäfer, Yuk Shan Cheng, Michael Debus, Derryck T. Reid, Kamalesh Dadi, Léa Bonhomme, I. Boisse, Madhusudan Malve, Mirsad Sarjlic, Michael Lehmitz, Omar Gabella
article en
3 citations

Abstract

The instrumentation plan for the ELT foresees the ArmazoNes high Dispersion Echelle Spectrograph (ANDES). The ANDES-project and consortium entered phase B in January 2022 and underwent several (internal and external) revisions by now to ensure that the requirements and eventually the challenging goals can be met by the physical design of the spectrograph. <br/> <br clear="all"/> Among its main scientific goals are the detection of atmospheres of exoplanets and the determination of fundamental physical constants. For this, high radial velocity precision and accuracy are required. Even though the ANDES-spectrograph is designed for maximum intrinsic stability, a calibration and thus a calibration unit is mandatory. To allow for maximum flexibility and modularity the calibration unit is physically split into three calibration units. <br/> <br clear="all"/> We show the design of the calibration units and their individual components, where possible. This includes the electronics, the mechanics, the software supporting and controlling the light guiding and calibration sources.

University of Bern (CH), Centre National de la Recherche Scientifique (FR), Laboratoire Univers et Particules de Montpellier (FR), University of Applied Sciences Emden Leer (DE), Max Planck Institute for Astronomy (DE), Observatoire Midi-Pyrénées (FR), Osservatorio Astronomico di Padova (IT), University of Göttingen (DE)
Science and Technology Facilities Council
Climate action
Openalex Percentile: Top 16%
Astronomy and Astrophysical Research
1.52
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