NIAOT OpenIR  > 中国科学院南京天文光学技术研究所  > 会议论文
The LAMOST middle resolution spectrograph
Hou Yonghui1,2,3; Tang Linlin1,2,3; Xu Mingming1,2,3; Jiang Haijiao1,2,3; Hu Zhongwen1,2,3; Wang Lei1,2,3; Ji Hangxin1,2,3; Zhu Yongtian1,2,3
2018-07-06
Conference NameSPIE Ground-based and Airborne Instrumentation for Astronomy VII(Vol.10702)
Source PublicationGround-based and Airborne Instrumentation for Astronomy VII
Conference Date2018-6-10
Conference PlaceAustin, Texas, United States
Abstract
The LAMOST completed its first five years of operation in June 2017, and 9 million low resolution spectra are obtained. The spectrographs have been upgraded in 2017, and the resolution can reach up to 7500(with 2/3 slit). In the midresolution mode, the wavelength can cover 495nm-535nm(blue band) and 630nm-680nm(red band). The LAMOST will carry out the middle resolution spectroscopic survey in September 2018, and 3 million middle resolution spectra will be obtained.

This paper describes the requirements, optical design and mechanical design of the LAMOST-MRS (the LAMOST middle resolution spectrograph).
KeywordSpectrograph Astronomical Instrumentation Optical Design Lamost
Subject Area天文技术与方法
Language英语
Document Type会议论文
Identifierhttp://ir.niaot.ac.cn/handle/114a32/1561
Collection中国科学院南京天文光学技术研究所_会议论文
天文光谱和高分辨成像技术研究室_会议论文
Affiliation1.南京天文光学技术研究所
2.天文光学技术重点实验室
3.中国科学院大学
Recommended Citation
GB/T 7714
Hou Yonghui,Tang Linlin,Xu Mingming,et al. The LAMOST middle resolution spectrograph[C],2018.
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