The development of ground-based infrared multi-object spectrograph based on the microshutter array

被引：0
|
作者：
Moon, Dae-Sik [1 ]
Sivanandam, Suresh [2 ]
Kutyrev, Alexander S. [3 ]
Moseley, Samuel H. [3 ]
Graham, James R. [4 ]
Roy, Aishwarya [5 ]
机构：
[1] Univ Toronto, Dept Astron, Toronto, ON M5S 3H4, Canada
[2] Univ Toronto, Dunlap Inst Astron & Astrophys, Toronto, ON M55 3H4, Canada
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[4] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[5] Indian Inst Technol Kharagpur, Dept Mech Engn, Kharagpur 721302, W Bengal, India
来源：
GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY V | 2014年 / 9147卷
关键词：
adaptive optics; infrared; micro-shutter array; multi-object; spectroscopy;
D O I：
10.1117/12.2057271
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We report on our development of a near-infrared multi-object spectrograph for ground-based applications using the micro-shutter array, which was originally developed for the Near Infrared Spectrograph of the James Webb Space Telescope. The micro-shutter array in this case acts as a source selector at a reimaged telescope focal plane. The developed spectrograph will be implemented either with ground-layer adaptive optics system or multi-conjugate adaptive optics system on a large telescope. This will enable for the first time fully reconfigurable infrared multi-object spectroscopy with adaptive optics systems. We envision studying diverse astronomical objects with our spectrograph, including high-redshift galaxies, galaxy clusters and super star clusters.
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页数：6
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