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The Antarctic Submillimetre Telescope

Published online by Cambridge University Press:  24 December 2009

L. Spinoglio ,
N. Epchtein ,
V. Minier ,
L. Olmi ,
G. Durand ,
E. Daddi ,
F. Israel ,
C. Kramer ,
P.-O. Lagage  and
M. de Petris
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V. Minier*
Affiliation:
CEA Saclay, Laboratoire AIM, Service d'Astrophysique/Irfu, France;
L. Olmi
Affiliation:
Osservatorio di Arcetri, INAF, Italy & University of Puerto Rico
G. Durand
Affiliation:
CEA Saclay, Laboratoire AIM, Service d'Astrophysique/Irfu, France;
E. Daddi
Affiliation:
CEA Saclay, Laboratoire AIM, Service d'Astrophysique/Irfu, France;
F. Israel
Affiliation:
Leiden observatory, The Netherlands
C. Kramer
Affiliation:
Universitaet zu Koeln, Germany & IRAM, Spain
P.-O. Lagage
Affiliation:
CEA Saclay, Laboratoire AIM, Service d'Astrophysique/Irfu, France;
M. de Petris
Affiliation:
La Sapienza, Rome, Italy
L. Sabbatini
Affiliation:
Dipartimento di Fisica, Roma 3, Italy
L. Spinoglio
Affiliation:
IFSI, INAF Roma, Italy
N. Schneider
Affiliation:
CEA Saclay, Laboratoire AIM, Service d'Astrophysique/Irfu, France;
N. Tothill
Affiliation:
Dept. of Physics, University of Exeter, Exeter, UK
P. Tremblin
Affiliation:
CEA Saclay, Laboratoire AIM, Service d'Astrophysique/Irfu, France;
L. Valenziano
Affiliation:
Universitaet zu Koeln, Germany & IRAM, Spain
C. Veyssière
Affiliation:
CEA Saclay, SIS/Irfu, France
*
vincent.minier@cea.fr
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Abstract

This report aims to provide a summary of the status of our Antarctic Submillimetre Telescope (AST) project up to date. It is a very new project for Antarctic astronomy. Necessary prerequisites for a future deployment of a large size telescope infrastructure have been tested in years 2007 and 2008. The knowledge of the transmission, frost formation and temperature gradient were fundamental parameters before starting a feasibility study. The telescope specifications and requirements are currently discussed with the industrial partnership.

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