English

MOSAIC: the high-multiplex and multi-IFU spectrograph for the ELT

Instrumentation and Methods for Astrophysics 2020-12-16 v1

Abstract

MOSAIC is the planned multi-object spectrograph for the 39m Extremely Large Telescope (ELT). Conceived as a multi-purpose instrument, it offers both high multiplex and multi-IFU capabilities at a range of intermediate to high spectral resolving powers in the visible and the near-infrared. MOSAIC will enable unique spectroscopic surveys of the faintest sources, from the oldest stars in the Galaxy and beyond to the first populations of galaxies that completed the reionisation of the Universe--while simultaneously opening up a wide discovery space. In this contribution we present the status of the instrument ahead of Phase B, showcasing the key science cases as well as introducing the updated set of top level requirements and the adopted architecture. The high readiness level will allow MOSAIC to soon enter the construction phase, with the goal to provide the ELT community with a world-class MOS capability as soon as possible after the telescope first light.

Keywords

Cite

@article{arxiv.2012.08393,
  title  = {MOSAIC: the high-multiplex and multi-IFU spectrograph for the ELT},
  author = {Rubén Sánchez-Janssen and Francois Hammer and Simon Morris and Jean-Gabriel Cuby and Lex Kaper and Matthias Steinmetz and Jose Afonso and Beatriz Barbuy and Edwin Bergin and Alexis Finoguenov and Jesús Gallego and Susan Kassin and Christopher Miller and Goran Östlin and Laura Pentericci and Daniel Schaerer and Bodo Ziegler and Fanny Chemla and Gavin Dalton and Fatima De Frondat and Chris Evans and David Le Mignant and Mathieu Puech and Myriam Rodrigues and Sylvestre Taburet and Lidia Tasca and Yanbin Yang and Sandrine Zanchetta and Timothy Butterley and Jean-Marc Conan and Kjetil Dohlen and Marc Dubbeldam and Kacem El Hadi and Annemieke Janssen and Thierry Fusco and Andreas Kelz and Marie Larrieu and Ian Lewis and Caroline Lim and Mike MacIntosh and Tim Morris and Ramon Navarro and Walter Seifert},
  journal= {arXiv preprint arXiv:2012.08393},
  year   = {2020}
}

Comments

Accepted to SPIE

R2 v1 2026-06-23T20:59:24.360Z