The ELT-MOS (MOSAIC)

Autor: Morris, S., Hammer, F., Jagourel, P., Evans, C.J., Puech, M., Dalton, G.B., Rodrigues, M., Sanchez-Janssen, R., Fitzsimons, E., Barbuy, B., Cuby, J.-G., Kaper, L., Roth, M., Rousset, G., Myers, R., Le Fèvre, O., Finogenov, A., Kotilainen, J., Castilho, B., Ostlin, G., Feltzing, S., Korn, A., Gallego, J., Castillo Morales, Á., Iglesias-Páramo, J., Pentericci, L., Ziegler, B., Afonso, J., Dubbledam, M., Close, M., Parr-Burman, P., Morris, T.J., Chemla, F., De Frondat, F., Kelz, A., Guinouard, I., Lewis, I.J., Middleton, K., Navarro, R., Larrieu, M., Pragt, J., Janssen, A., Dohlen, K., El Hadi, K., Gendron, É., Yang, Y., Wells, M., Conan, J.-M., Fusco, T., Schaerer, D., Bergin, E., Taburet, S., Frotin, M., Berkourn, N., Simard, L., Takami, H.
Přispěvatelé: Department of Physics [Durham University], Durham University, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), ​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​​ISIS Neutron and Muon Source (ISIS), STFC Rutherford Appleton Laboratory (RAL), Science and Technology Facilities Council (STFC)-Science and Technology Facilities Council (STFC), Universidade de São Paulo (USP), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Universiteit van Amsterdam (UvA), Leibniz-Institut für Astrophysik Potsdam (AIP), University of Helsinki, Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Laboratorio Nacional de Astrofisica, Oskar Klein Centre [Stockholm], Stockholm University, Lund University [Lund], Uppsala University, Universidad Complutense de Madrid = Complutense University of Madrid [Madrid] (UCM), Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), INAF - Osservatorio Astronomico di Roma (OAR), Istituto Nazionale di Astrofisica (INAF), Universität Wien, Observatório Astronómico de Lisboa, University of Oxford [Oxford], Netherlands Research School for Astronomy, Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), DOTA, ONERA, Université Paris Saclay (COmUE) [Châtillon], ONERA-Université Paris Saclay (COmUE), Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève (UNIGE), University of Michigan [Ann Arbor], University of Michigan System, High Energy Astrophys. & Astropart. Phys (API, FNWI), Universidade de São Paulo = University of São Paulo (USP), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Helsingin yliopisto = Helsingfors universitet = University of Helsinki, University of Oxford, Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université de Genève = University of Geneva (UNIGE)
Jazyk: angličtina
Rok vydání: 2018
Předmět:
Zdroj: E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Digital.CSIC. Repositorio Institucional del CSIC
instname
SPIE Astronomical Telescopes + Instrumentation
SPIE Astronomical Telescopes + Instrumentation, Jun 2018, Austin, United States. ⟨10.1117/12.2311430⟩
Ground-based and Airborne Instrumentation for Astronomy VII: 10-14 June 2018, Austin, Texas, United States, 1
E-Prints Complutense. Archivo Institucional de la UCM
ISSN: 0277-786X
DOI: 10.1117/12.2311430⟩
Popis: When combined with the huge collecting area of the ELT, MOSAIC will be the most effective and flexible Multi-Object Spectrograph (MOS) facility in the world, having both a high multiplex and a multi-Integral Field Unit (Multi-IFU) capability. It will be the fastest way to spectroscopically follow-up the faintest sources, probing the reionisation epoch, as well as evaluating the evolution of the dwarf mass function over most of the age of the Universe. MOSAIC will be world-leading in generating an inventory of both the dark matter (from realistic rotation curves with MOAO fed NIR IFUs) and the cool to warm-hot gas phases in z=3.5 galactic haloes (with visible wavelenth IFUs). Galactic archaeology and the first massive black holes are additional targets for which MOSAIC will also be revolutionary. MOAO and accurate sky subtraction with fibres have now been demonstrated on sky, removing all low Technical Readiness Level (TRL) items from the instrument. A prompt implementation of MOSAIC is feasible, and indeed could increase the robustness and reduce risk on the ELT, since it does not require diffraction limited adaptive optics performance. Science programmes and survey strategies are currently being investigated by the Consortium, which is also hoping to welcome a few new partners in the next two years.
6 pages, 3 figures, Submitted to SPIE Proceedings, AS18
Databáze: OpenAIRE
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