iSHELL: a construction, assembly and testing
iSHELL: a construction, assembly and testing
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iSHELL：构建、组装和测试
DOI：
10.1117/12.2232064
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发表时间：
2016
期刊：
影响因子：
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通讯作者：
Eric A. Warmbier
中科院分区：
文献类型：
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作者：
J. Rayner;A. Tokunaga;D. Jaffe;Morgan B. Bonnet;G. Ching;M. Connelley;Dan Kokubun;C. Lockhart;Eric A. Warmbier
iSHELL是为位于夏威夷Maunakea的NASA红外望远镜设施建造的1.10-5.3 μm高光谱分辨率摄谱仪。色散是用硅浸没光栅完成的，以保持仪器足够小，可以安装在望远镜的卡塞格伦焦点上。白色光瞳摄谱仪产生高达R= 75，000的分辨能力。交叉色散光栅安装在一个可倾斜的机制允许观察者选择不同的波长范围，并结合狭缝轮和德克尔机制，狭缝长度范围从5英寸到25英寸。一个Teledyne 2048 × 2048夏威夷2 RG阵列用于光谱仪，一个Raytheon 512 × 512 Aladdin 2阵列用于狭缝观察器，用于物体采集和引导。预计2016年年中将出现第一束光。在本文中，我们讨论的建设，组装和实验室测试的细节。
iSHELL is 1.10-5.3 μm high spectral resolution spectrograph being built for the NASA Infrared Telescope Facility on Maunakea, Hawaii. Dispersion is accomplished with a silicon immersion grating in order to keep the instrument small enough to be mounted at the Cassegrain focus of the telescope. The white pupil spectrograph produces resolving powers of up to R=75,000. Cross-dispersing gratings mounted in a tilt-able mechanism allow observers to select different wavelength ranges and, in combination with a slit wheel and Dekker mechanism, slit lengths ranging from 5ʺ″ to 25ʺ″. One Teledyne 2048x2048 Hawaii 2RG array is used in the spectrograph, and one Raytheon 512x512 Aladdin 2 array is used in a slit viewer for object acquisition and guiding. First light is expected in mid-2016. In this paper we discuss details of the construction, assembly and laboratory testing.