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The Science Case for Multi-Object Spectroscopy on the European ELT

Authors :
Evans, Chris
Puech, Mathieu
Afonso, Jose
Almaini, Omar
Amram, Philippe
Aussel, Hervé
Barbuy, Beatriz
Basden, Alistair
Bastian, Nate
Battaglia, Giuseppina
Biller, Beth
Bonifacio, Piercarlo
Bouché, Nicholas
Bunker, Andy
Caffau, Elisabetta
Charlot, Stephane
Cirasuolo, Michele
Clenet, Yann
Combes, Francoise
Conselice, Chris
Contini, Thierry
Cuby, Jean-Gabriel
Dalton, Gavin
Davies, Ben
de Koter, Alex
Disseau, Karen
Dunlop, Jim
Epinat, Benoît
Fiore, Fabrizio
Feltzing, Sofia
Ferguson, Annette
Flores, Hector
Fontana, Adriano
Fusco, Thierry
Gadotti, Dimitri
Gallazzi, Anna
Gallego, Jesus
Giallongo, Emanuele
Gonçalves, Thiago
Gratadour, Damien
Guenther, Eike
Hammer, Francois
Hill, Vanessa
Huertas-Company, Marc
Ibata, Roridgo
Kaper, Lex
Korn, Andreas
Larsen, Søren
Fèvre, Olivier Le
Lemasle, Bertrand
Maraston, Claudia
Mei, Simona
Mellier, Yannick
Morris, Simon
Östlin, Göran
Paumard, Thibaut
Pello, Roser
Pentericci, Laura
Peroux, Celine
Petitjean, Patrick
Rodrigues, Myriam
Rodríguez-Muñoz, Lucía
Rouan, Daniel
Sana, Hugues
Schaerer, Daniel
Telles, Eduardo
Trager, Scott
Tresse, Laurence
Welikala, Niraj
Zibetti, Stefano
Ziegler, Bodo
Publication Year :
2015

Abstract

This White Paper presents the scientific motivations for a multi-object spectrograph (MOS) on the European Extremely Large Telescope (E-ELT). The MOS case draws on all fields of contemporary astronomy, from extra-solar planets, to the study of the halo of the Milky Way and its satellites, and from resolved stellar populations in nearby galaxies out to observations of the earliest 'first-light' structures in the partially-reionised Universe. The material presented here results from thorough discussions within the community over the past four years, building on the past competitive studies to agree a common strategy toward realising a MOS capability on the E-ELT. The cases have been distilled to a set of common requirements which will be used to define the MOSAIC instrument, entailing two observational modes ('high multiplex' and 'high definition'). When combined with the unprecedented sensitivity of the E-ELT, MOSAIC will be the world's leading MOS facility. In analysing the requirements we also identify a high-multiplex MOS for the longer-term plans for the E-ELT, with an even greater multiplex (>1000 targets) to enable studies of large-scale structures in the high-redshift Universe. Following the green light for the construction of the E-ELT the MOS community, structured through the MOSAIC consortium, is eager to realise a MOS on the E-ELT as soon as possible. We argue that several of the most compelling cases for ELT science, in highly competitive areas of modern astronomy, demand such a capability. For example, MOS observations in the early stages of E-ELT operations will be essential for follow-up of sources identified by the James Webb Space Telescope (JWST). In particular, multi-object adaptive optics and accurate sky subtraction with fibres have both recently been demonstrated on sky, making fast-track development of MOSAIC feasible.<br />Comment: Significantly expanded and updated version of previous ELT-MOS White Paper, so there is some textual overlap with arXiv:1303.0029

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.1501.04726
Document Type :
Working Paper