Science case and requirements for the MOSAIC concept for a multi-object spectrograph for the European Extremely Large Telescope

Author(s)
Chris J. Evans, M Puech, B Barbuy, Bodo Ziegler
Abstract

Over the past 18 months we have revisited the science requirements for a multi-object spectrograph (MOS) for the European Extremely Large Telescope (E-ELT). These efforts span the full range of E-ELT science and include input from a broad cross-section of astronomers across the ESO partner countries. In this contribution we summarise the key cases relating to studies of high-redshift galaxies, galaxy evolution, and stellar populations, with a more expansive presentation of a new case relating to detection of exoplanets in stellar clusters. A general requirement is the need for two observational modes to best exploit the large (≥40 arcmin

2) patrol field of the E-ELT. The first mode ('high multiplex') requires integrated-light (or coarsely resolved) optical/near-IR spectroscopy of >100 objects simultaneously. The second ('high definition'), enabled by wide-field adaptive optics, requires spatially-resolved, near-IR of >10 objects/sub-fields. Within the context of the conceptual study for an ELT-MOS called MOSAIC, we summarise the toplevel requirements from each case and introduce the next steps in the design process.

Organisation(s)
Department of Astrophysics
External organisation(s)
Université Paris VII - Paris-Diderot, Instituto Oceanográfico, UK Astronomy Technology Centre, The Royal Observatory, Edinburgh
No. of pages
17
DOI
https://doi.org/10.1117/12.2055857
Publication date
07-2014
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
ASJC Scopus subject areas
Electronic, Optical and Magnetic Materials, Condensed Matter Physics, Applied Mathematics, Electrical and Electronic Engineering, Computer Science Applications
Portal url
https://ucrisportal.univie.ac.at/en/publications/e1be1961-72ea-4e81-88d8-c351967b6adf