MAX38: A Mid-infrared Camera for Ground-based Observations at 8 to 38 Microns

被引：0

作者：

Miyata, T. ^{[1
]}

Sako, S. ^{[1
]}

Nakamura, T. ^{[1
]}

Onaka, T. ^{[2
]}

Kataza, H. ^{[3
]}

机构：

[1] Osawa 2-21-1, Tokyo 1810015, Japan

[2] Bunkyo ku, Hongo 7-3-1, Tokyo 1130033, Japan

[3] 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2298510, Japan

来源：

EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY | 2009年 / 1158卷

关键词：

Mid infrared; Instrumentation; Groundbased telescopes; LATEX 2(epsilon);

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We are developing a new infrared camera - MAX38 (Mid-infrared Astronomical eXplorer) - for ground-based mid-infrared (8-38 microns) observations. This spectral region will be very important for the study of planetary disks. The MAX38 will be attached on the University of Tokyo Atacama 1.0-meter telescope, which is the world's highest infrared telescope, at the summit of Co. Chajnantor (altitude 5,640 meters), in Chile's Atacama Desert. Thanks to the high altitude and dry weather condition of the site we can access the 30-micron wavelength region from ground-based telescopes for the first time.

引用

页码：395 / +

页数：2

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