THE ANTARCTIC SUBMILLIMETRE TELESCOPE

被引：2

作者：

Minier, V. ^{[1
]}

Olmi, L. ^{[2
,3
]}

Durand, G. ^{[1
]}

Daddi, E. ^{[1
]}

Israel, F. ^{[4
]}

Kramer, C. ^{[5
,6
]}

Lagage, P-O ^{[1
]}

de Petris, M. ^{[7
]}

Sabbatini, L. ^{[8
]}

Spinogho, L. ^{[9
]}

Schneider, N. ^{[1
]}

Tothill, N. ^{[10
]}

Tremblin, P. ^{[1
]}

Valenziano, L. ^{[5
,6
]}

Veyssiere, C. ^{[11
]}

机构：

[1] CEA Saclay, Lab AIM, Serv Astrophys Irfu, Gif Sur Yvette, France

[2] INAF, Osservatorio Arcetri, Rome, Italy

[3] Univ Puerto Rico, San Juan, PR 00936 USA

[4] Leiden Observ, Leiden, Netherlands

[5] Univ Cologne, Cologne, Germany

[6] IRAM, Barcelona, Spain

[7] La Sapienza, Rome, Italy

[8] Dipartimento Fis, Rome 3, Italy

[9] INAF Roma, IFSI, Rome, Italy

[10] Univ Exeter, Dept Phys, Exeter, Devon, England

[11] CEA Saclay, SIS Irfu, Gif Sur Yvette, France

来源：

3RD ARENA CONFERENCE ON AN ASTRONOMICAL OBSERVATORY AT CONCORDIA (DOME C, ANTARCTICA) | 2009年 / 40卷

基金：

美国国家科学基金会;

关键词：

D O I：

10.1051/eas/1040039

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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

引用

页码：269 / +

页数：2

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