Near IR arrays for ground-based and space-based astronomy

被引：15

作者：

Hoffman, AW ^{[1
]}

Ando, KJ ^{[1
]}

Estrada, AD ^{[1
]}

Garnett, JD ^{[1
]}

Lum, NA ^{[1
]}

Love, PJ ^{[1
]}

Rosbeck, JP ^{[1
]}

Sparkman, KP ^{[1
]}

Fowler, AM ^{[1
]}

Pipher, J ^{[1
]}

Forrest, W ^{[1
]}

机构：

[1] Santa Barbara Res Ctr, Raytheon, Goleta, CA 93117 USA

来源：

INFRARED ASTRONOMICAL INSTRUMENTATION, PTS 1-2 | 1998年 / 3354卷

关键词：

infrared astronomy; infrared arrays; InSb; HgCdTe; SIRTF; IRIS; NGST; VIRTIS; Raytheon; SBRC;

D O I：

10.1117/12.317271

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This paper is a review of current astronomy projects at Raytheon/SBRC in the near-infrared (IR) band (optical to 5 mu m). Another paper in this same session (3354-11) covers astronomy projects in longer wavelengths. For ground-based astronomy, InSb arrays with formats of 256 x 256, 512 x 512, and 1024 x 1024 have been developed and tested. For space-based astronomy, four projects are discussed with array formats ranging from 256 x 256 to 2K x 2K. The space projects support instruments on the SIRTF, IRIS, NGST, and Rosetta missions. Representative data are presented from 1024 x 1024 and 256 x 256 arrays obtained by test facilities at NOAO and the University of Rochester.

引用

页码：24 / 29

页数：6