The Infrared Camera and Spectrograph for the Subaru Telescope

被引：121
作者：
Tokunaga, AT [1 ]
Kobayashi, N [1 ]
Bell, J [1 ]
Ching, G [1 ]
Hodapp, K [1 ]
Hora, J [1 ]
Neill, D [1 ]
Onaka, P [1 ]
Rayner, J [1 ]
Robertson, L [1 ]
Warren, DW [1 ]
Weber, M [1 ]
Young, T [1 ]
机构：
[1] Univ Hawaii, Astron Inst, Honolulu, HI 96822 USA
来源：
INFRARED ASTRONOMICAL INSTRUMENTATION, PTS 1-2 | 1998年 / 3354卷
关键词：
infrared; camera; spectrograph; Subaru Telescope;
D O I：
10.1117/12.317277
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A 1-5 mu m Infrared Camera and Spectrograph (IRCS) is described. The IRCS will be a facility instrument for the 8.2 m Subaru Telescope at Mauna Kea. It consists of two sections, a spectrograph and a camera section. The spectrograph is a cross-dispersed echelle that will provide a resolving power (lambda/Delta lambda) of 20,000 with a slit width of 0.15 arcsec and two-pixel sampling. The camera section serves as a slit viewer and as a camera with two pixel scales, 0.022 arcsec/pixel and 0.060 arcsec/pixel. Grisms providing 400-1400 resolving power will be available. Each section will utilize an ALADDIN II 1024x1024 InSb array. The instrument specifications are optimized for 2.2 mu m using the adaptive optics and the tip-tilt secondary systems of the Subaru Telescope.
引用
收藏
页码：512 / 524
页数：13
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