MOSAIC at the ELT: a unique instrument for the largest ground-based telescope

Open Access
Authors
Publication date 2024
Host editors
  • J.J. Bryant
  • K. Motohara
  • J.R. Vernet
Book title Ground-based and Airborne Instrumentation for Astronomy X
Book subtitle 16–21 June 2024, Yokohama, Japan
ISBN
  • 9781510675155
ISBN (electronic)
  • 9781510675162
Series Proceedings of SPIE
Event SPIE: Astronomical Telescopes + Instrumentation
Article number 13096 15
Volume | Issue number 1
Number of pages 10
Publisher Bellingham: SPIE
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
MOSAIC is the Multi-Object Spectrograph (MOS) for the 39m Extremely Large Telescope (ELT) of the European Southern Observatory (ESO), with unique capabilities in terms of multiplex, wavelength coverage and spectral resolution. It is a versatile multi-object spectrograph working in both the Visible and NIR domains, designed to cover the largest possible area (∼40 arcmin2) on the focal plane, and optimized to achieve the best possible signal-to-noise ratio on the faintest sources, from stars in our Galaxy to galaxies at the epoch of the reionization. In this paper we describe the main characteristics of the instrument, including its expected performance in the different observing modes. The status of the project will be briefly presented, together with the positioning of the instrument in the landscape of the ELT instrumentation. We also review the main expected scientific contributions of MOSAIC, focusing on the synergies between this instrument and other major ground-based and space facilities.
Document type Conference contribution
Language English
Published at https://doi.org/10.1117/12.3019047
Downloads
MOSAIC at the ELT (Final published version)
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