Trade-offs in the visible spectrograph of the ELT instrument MOSAIC

Authors
  • A.W. Janssen
  • E. Sokolova
  • J. Pragt
  • J. Kragt
  • R. Navarro
  • N. Tromp
  • E. Fitzsimons
  • M. Rodrigues
  • M. Larrieu
  • A. Kelz
  • T. Morris
  • P. Jagourel
  • F. Chemla
  • L. Kaper
  • G. Dalton
Publication date 2018
Host editors
  • C.J. Evans
  • L. Simard
  • H. Takami
Book title Ground-based and Airborne Instrumentation for Astronomy VII
Book subtitle 10-14 June 2018, Austin, Texas, United States
ISBN
  • 9781510619579
ISBN (electronic)
  • 9781510619586
Series Proceedings of the SPIE
Event Ground-based and Airborne Instrumentation for Astronomy VII
Article number 107029F
Volume | Issue number 5
Number of pages 7
Publisher Bellingham, WA: SPIE
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
MOSAIC is a concept for a multi-object spectrograph for the Extremely Large Telescope (ELT). It is planned to cover the wavelength range from 460 nm to 1800 nm with 5 visible spectrographs and 5 near-infrared spectrographs. The ELT is far from diffraction limited in the visible wavelength range. Rather than developing a large and complex AO system, it was decided that the instrument will be seeing limited in the visible. Spot sizes are therefore about 2.8 mm in diameter in the ELT focal plane, and need to be sampled by multiple fibers with large core diameter. As a result, large optics is required to achieve the science requirements on spectral resolution, bandwidth and multiplex. We work in close collaboration with manufacturers to design an instrument that is feasible and meets the scientific requirements.
Document type Conference contribution
Language English
Published at https://doi.org/10.1117/12.2313302
Other links http://adsabs.harvard.edu/abs/2018SPIE10702E..9FJ
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