Adaptive optics for the 6.5 m MMT

被引：17

作者：

Lloyd-Hart, M ^{[1
]}

Wildi, F ^{[1
]}

Martin, H ^{[1
]}

McGuire, P ^{[1
]}

Kenworthy, M ^{[1
]}

Johnson, R ^{[1
]}

Fitz-Patrick, B ^{[1
]}

Angeli, G ^{[1
]}

Miller, S ^{[1
]}

Angel, R ^{[1
]}

机构：

[1] Univ Arizona, Ctr Astron Adapt Opt, Tucson, AZ 85721 USA

来源：

ADAPTIVE OPTICAL SYSTEMS TECHNOLOGY, PTS 1 AND 2 | 2000年 / 4007卷

关键词：

D O I：

10.1117/12.390307

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The adaptive optics system for the 6.5 m MMT conversion telescope will be the first to compensate the aberrated wavefront at the telescope's secondary mirror. This approach has unique advantages in terms of optical simplicity, high throughput and low emissivity. We report here the present state of construction, and the results of static acid dynamic performance tests of the Cassegrain optical package.

引用

页码：167 / 174

页数：8