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A Wide-field, Optical/Infrared, 2.5 m class Telescope for Antarctica

Published online by Cambridge University Press:  24 December 2009

M.G. Burton
Affiliation:
School of Physics, University of New South Wales, Australia
D. Burgarella
Affiliation:
Observatoire Astronomique de Marseille Provence, Université d'Aix-Marseille, France
M. Andersen
Affiliation:
Københavns Universitet, Dennmark
M. Busso
Affiliation:
Università degli Studi di Perugia, Italy
C. Eiroa
Affiliation:
Universidad Autónoma de Madrid, Spain
N. Epchtein
Affiliation:
CNRA–Fizeau, Université de Nice Sophia Antipolis, France
J.-P. Maillard
Affiliation:
Institut d'Astrophysique de Paris, France
P. Persi
Affiliation:
Istituto di Astrofisica Spaziale e Fisica Cosmica, Italy
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Abstract

This report provides the recommendations of ARENA Working Group 1 concerning the development of and objectives for a wide-field, optical/infrared, 2.5 m class telescope for Antarctica. It discusses the key science drivers for such a telescope, the performance and capabilities it should have, and the logistics and infrastructure issues relevant to its construction and operation.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2010

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