The IRAIT project - Infrared astronomy from Antarctica

被引：3

作者：

Busso, M ^{[1
]}

Tosti, G ^{[1
]}

Roncella, F ^{[1
]}

Bagaglia, M ^{[1
]}

Nucciarelli, G ^{[1
]}

Fastellini, R ^{[1
]}

Straniero, O ^{[1
]}

Dolci, M ^{[1
]}

Ragni, M ^{[1
]}

Di Varano, I ^{[1
]}

Corcione, L ^{[1
]}

Abia, C ^{[1
]}

Dominguez, I ^{[1
]}

Rossi, F ^{[1
]}

Nicolini, A ^{[1
]}

机构：

[1] Univ Perugia, Dept Phys, I-06100 Perugia, Italy

来源：

Dome C: Astronomy and Astrophysics Meeting | 2005年 / 14卷

关键词：

D O I：

10.1051/eas:2005028

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Concordia Station (Candidi 2003), on the Antarctica Plateau, will soon become one of the best observatories to perform infrared observations in the 2-20 mu m atmospheric windows and beyond, thanks to its low sky background, low temperature and high atmospheric transparency. The possibility of passively cooling the telescope is a further advantage. We describe here the first permanent Antarctic infrared telescope, under development for the Dome C base. It is the International Robotic Antarctic Infrared Telescope (IRAIT). We briefly outline a few scientific motivations for it, then we review the technical characteristics and the status of its development. The infrared camera for IRAIT is described in another dedicated paper in this volume.

引用

页码：181 / 186

页数：6

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