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Title:
EELT-HIRES the high-resolution spectrograph for the E-ELT
Authors:
Marconi, A.; Di Marcantonio, P.; D'Odorico, V.; Cristiani, S.; Maiolino, R.; Oliva, E.; Origlia, L.; Riva, M.; Valenziano, L.; Zerbi, F. M.; Abreu, M.; Adibekyan, V.; Allende Prieto, C.; Amado, P. J.; Benz, W.; Boisse, I.; Bonfils, X.; Bouchy, F.; Buchhave, L.; Buscher, D.; Cabral, A.; Canto Martins, B. L.; Chiavassa, A.; Coelho, J.; Christensen, L. B.; Delgado-Mena, E.; de Medeiros, J. R.; Di Varano, I.; Figueira, P.; Fisher, M.; Fynbo, J. P. U.; Glasse, A. C. H.; Haehnelt, M.; Haniff, C.; Hansen, C. J.; Hatzes, A.; Huke, P.; Korn, A. J.; Leão, I. C.; Liske, J.; Lovis, C.; Maslowski, P.; Matute, I.; McCracken, R. A.; Martins, C. J. A. P.; Monteiro, M. J. P. F. G.; Morris, S.; Morris, T.; Nicklas, H.; Niedzielski, A.; Nunes, N. J.; Palle, E.; Parr-Burman, P. M.; Parro, V.; Parry, I.; Pepe, F.; Piskunov, N.; Queloz, D.; Quirrenbach, A.; Rebolo Lopez, R.; Reiners, A.; Reid, D. T.; Santos, N.; Seifert, W.; Sousa, S.; Stempels, H. C.; Strassmeier, K.; Sun, X.; Udry, S.; Vanzi, L.; Vestergaard, M.; Weber, M.; Zackrisson, E.
Affiliation:
AA(Univ. degli Studi di Firenze (Italy)), AB(INAF - Osservatorio Astronomico di Trieste (Italy)), AC(INAF - Osservatorio Astronomico di Trieste (Italy)), AD(INAF - Osservatorio Astronomico di Trieste (Italy)), AE(Univ. of Cambridge (United Kingdom)), AF(INAF - Osservatorio Astrofisico di Arcetri (Italy)), AG(INAF - Osservatorio Astronomico di Bologna (Italy)), AH(INAF - Osservatorio Astronomico di Brera (Italy)), AI(INAF - IASF Bologna (Italy)), AJ(Istituto Nazionale di Astrofisica (Italy)), AK(Univ. de Lisboa (Portugal)), AL(Univ. do Porto (Portugal)), AM(Instituto de Astrofísica de Canarias (Spain)), AN(Instituto de Astrofísica de Andalucía (Spain)), AO(Univ. of Bern (Switzerland)), AP(Lab. d'Astrophysique de Marseille (France)), AQ(Observatoire de Science de l'Univ. de Grenoble (France)), AR(Univ. de Genève (Switzerland)), AS(Univ. of Copenhagen (Denmark)), AT(Univ. of Cambridge (United Kingdom)), AU(Univ. de Lisboa (Portugal)), AV(Federal Univ. of Rio Grande do Norte (Brazil)), AW(Lab. Lagrange, Univ. Côte d'Azur, Observatoire de la Côte d'Azur (France)), AX(Univ. de Lisboa (Portugal)), AY(Dark Cosmology Ctr. (Denmark)), AZ(Univ. do Porto (Portugal)), BA(Univ. Federal of Rio Grande do Norte (Brazil)), BB(Leibniz-Institut für Astrophysik Potsdam (Germany)), BC(Univ. do Porto (Portugal)), BD(Univ. of Cambridge (United Kingdom)), BE(Dark Cosmology Ctr. (Denmark)), BF(UK Astronomy Technology Ctr. (United Kingdom)), BG(Univ. of Cambridge (United Kingdom)), BH(Univ. of Cambridge (United Kingdom)), BI(Dark Cosmology Ctr. (Denmark)), BJ(Thüringer Landessternwarte Tautenburg (Germany)), BK(Univ. of Göttingen (Germany)), BL(Uppsala Univ. (Sweden)), BM(Federal Univ. of Rio Grande do Norte (Brazil)), BN(Univ. Hamburg (Germany)), BO(Univ. de Genève (Switzerland)), BP(Nicolaus Copernicus Univ. (Poland)), BQ(Univ. de Lisboa (Portugal)), BR(Heriot Watt Univ. (United Kingdom)), BS(Univ. do Porto (Portugal)), BT(Univ. do Porto (Portugal)), BU(Durham Univ. (United Kingdom)), BV(Durham Univ. (United Kingdom)), BW(Univ. of Göttingen (Germany)), BX(Nicolaus Copernicus Univ. (Poland)), BY(Univ. de Lisboa (Portugal)), BZ(Instituto de Astrofísica de Canarias (Spain)), CA(UK Astronomy Technology Ctr. (United Kingdom)), CB(Instituto Mauá de Tecnologia (Brazil)), CC(Univ. of Cambridge (United Kingdom)), CD(Univ. de Genève (Switzerland)), CE(Uppsala Univ. (Sweden)), CF(Univ. of Cambridge (United Kingdom)), CG(Univ. Heidelberg (Germany)), CH(Instituto de Astrofísica de Canarias (Spain)), CI(Univ. of Göttingen (Germany)), CJ(Heriot Watt Univ. (United Kingdom)), CK(Univ. do Porto (Portugal)), CL(Univ. Heidelberg (Germany)), CM(Univ. do Porto (Portugal)), CN(Uppsala Univ. (Sweden)), CO(Leibniz-Institut für Astrophysik Potsdam (Germany)), CP(Univ. of Cambridge (United Kingdom)), CQ(Univ. de Genève (Switzerland)), CR(Pontificia Univ. Católica de Chile (Chile)), CS(Dark Cosmology Ctr. (Denmark)), CT(Leibniz-Institut für Astrophysik Potsdam (Germany)), CU(Uppsala Univ. (Sweden))
Publication:
Proceedings of the SPIE, Volume 9908, id. 990823 12 pp. (2016). (SPIE Homepage)
Publication Date:
08/2016
Origin:
SPIE
Abstract Copyright:
(c) 2016: SPIE. Downloading of the abstract is permitted for personal use only.
Comment:
ISBN: 9781510601956
DOI:
10.1117/12.2231653
Bibliographic Code:
2016SPIE.9908E..23M

Abstract

The first generation of E-ELT instruments will include an optic-infrared High Resolution Spectrograph, conventionally indicated as EELT-HIRES, which will be capable of providing unique breakthroughs in the fields of exoplanets, star and planet formation, physics and evolution of stars and galaxies, cosmology and fundamental physics. A 2-year long phase A study for EELT-HIRES has just started and will be performed by a consortium composed of institutes and organisations from Brazil, Chile, Denmark, France, Germany, Italy, Poland, Portugal, Spain, Sweden, Switzerland and United Kingdom. In this paper we describe the science goals and the preliminary technical concept for EELT-HIRES which will be developed during the phase A, as well as its planned development and consortium organisation during the study.
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