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iSHELL: a 1-5 micron cross-dispersed R=70,000 immersion grating spectrograph for IRTF

机译:Ishell:1-5微米交叉分散r = 70,000浸泡光栅光谱仪,用于irtf

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iSHELL is 1.15-5.4 μm high spectral resolution spectrograph being built for the NASA Infrared Telescope Facility onMauna Kea, Hawaii. Dispersion is accomplished with silicon immersion gratings in order to keep the instrument smallenough to be mounted at the Cassegrain focus of the telescope. The white pupil spectrograph is designed to produceresolving powers of up to R=70,000. Cross-dispersing gratings mounted in a tilt-able mechanism at the second pupilallow observers to select different wavelength ranges and, in combination with a slit wheel and dekker mechanism, slitlengths ranging from 5″ to 25″. One Teledyne 2048x2048 Hawaii 2RG array is used in the spectrograph, and oneRaytheon 512x512 Aladdin 2 array is used in a slit viewer for object acquisition, guiding, and imaging. About $4 millionin funding has been provided by NSF, NASA and the University of Hawaii. First light is expected in about 2015. In thispaper we discuss the science drivers, instrument design and expected performance.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:ISHELL是1.15-5.4μ M高光谱分辨率光谱仪,为NASA红外望远镜设施Onmauna Kea,夏威夷建造。通过硅浸渍光栅完成分散,以保持仪器少量安装在望远镜的Cassegrain焦点上。白色瞳孔光谱仪设计为生产高达r = 70,000的能力。在第二瞳孔观察者处安装在第二瞳孔观察者的倾斜机构的交叉分散光栅,以选择不同的波长范围,以及与狭缝和达克斯机构的组合,从5&#8243的缝隙长度;到25″一个Teledyne 2048x2048夏威夷2RG阵列用于光谱仪,oneraytheon 512x512 Aladdin 2阵列用于狭缝观众,用于对象采集,引导和成像。 NSF,NASA和夏威夷大学提供约4000万美元的资金。预计大约2015年的第一盏灯仅供个人使用的摘要下载。

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