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

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 wil...

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المؤلفون الرئيسيون: Dalton, GB, Sánchez-Janssen, R, Hammer, F, Morris, S, Cuby, J-G, Kaper, L, Steinmetz, M, Afonso, J, Barbuy, B, Rodrigues, M, Lewis, I, Bergin, E, Evans, C
التنسيق: Journal article
اللغة:English
منشور في: Society of Photo-optical Instrumentation Engineers 2020
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author Dalton, GB
Sánchez-Janssen, R
Hammer, F
Morris, S
Cuby, J-G
Kaper, L
Steinmetz, M
Afonso, J
Barbuy, B
Rodrigues, M
Lewis, I
Bergin, E
Evans, C
author_facet Dalton, GB
Sánchez-Janssen, R
Hammer, F
Morris, S
Cuby, J-G
Kaper, L
Steinmetz, M
Afonso, J
Barbuy, B
Rodrigues, M
Lewis, I
Bergin, E
Evans, C
author_sort Dalton, GB
collection OXFORD
description 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.
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spelling oxford-uuid:bd9ab50b-db6a-420f-aeb5-68ea1873248d2022-03-27T05:33:03ZMOSAIC: the high multiplex and multi-IFU spectrograph for the ELTJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:bd9ab50b-db6a-420f-aeb5-68ea1873248dEnglishSymplectic ElementsSociety of Photo-optical Instrumentation Engineers2020Dalton, GBSánchez-Janssen, RHammer, FMorris, SCuby, J-GKaper, LSteinmetz, MAfonso, JBarbuy, BRodrigues, MLewis, IBergin, EEvans, CMOSAIC 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.
spellingShingle Dalton, GB
Sánchez-Janssen, R
Hammer, F
Morris, S
Cuby, J-G
Kaper, L
Steinmetz, M
Afonso, J
Barbuy, B
Rodrigues, M
Lewis, I
Bergin, E
Evans, C
MOSAIC: the high multiplex and multi-IFU spectrograph for the ELT
title MOSAIC: the high multiplex and multi-IFU spectrograph for the ELT
title_full MOSAIC: the high multiplex and multi-IFU spectrograph for the ELT
title_fullStr MOSAIC: the high multiplex and multi-IFU spectrograph for the ELT
title_full_unstemmed MOSAIC: the high multiplex and multi-IFU spectrograph for the ELT
title_short MOSAIC: the high multiplex and multi-IFU spectrograph for the ELT
title_sort mosaic the high multiplex and multi ifu spectrograph for the elt
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