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Title:
The LAMOST middle resolution spectrograph
Author: Hou, YongHui(候永辉)1,2,3; Tang LinLin(唐琳琳)1,2,3; Xu MingMing(许明明)1,2,3; Jiang, HaiJiao(姜海娇)1,2,3; Hu, ZhongWen(胡中文)1,2,3; Wang, Lei(王磊)1,2,3; Ji, HangXin(季杭馨)1,2,3; Zhu, YongTian(朱永田)1,2,3
Issued Date: 2018-07-06
Conference Name: SPIE Ground-based and Airborne Instrumentation for Astronomy VII(Vol.10702)
Conference Date: 2018-6-10
Conference Place: Austin, Texas, United States
Keyword: Spectrograph ; Astronomical Instrumentation ; Optical Design ; LAMOST
Subject: 天文技术与方法
English 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).
Source: Ground-based and Airborne Instrumentation for Astronomy VII
Language: 英语
Content Type: 会议论文
URI: http://ir.niaot.ac.cn/handle/114a32/1561
Appears in Collections:中科院南京天光所知识成果_会议论文
天文光谱和高分辨成像技术研究室_会议论文

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description.institution: 1.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:
Hou Yonghui,Tang Linlin,Xu Mingming,et al. The LAMOST middle resolution spectrograph[C]. 见:SPIE Ground-based and Airborne Instrumentation for Astronomy VII(Vol.10702). Austin, Texas, United States. 2018-6-10.
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