Presentation + Paper
6 July 2018 The LAMOST middle resolution spectrograph
Author Affiliations +
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)
Conference Presentation
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Yonghui Hou, Linlin Tang, Mingming Xu, Haijiao Jiang, Zhongwen Hu, Lei Wang, Hangxin Ji, and Yongtian Zhu "The LAMOST middle resolution spectrograph", Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 107021I (6 July 2018); https://doi.org/10.1117/12.2312279
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CITATIONS
Cited by 2 scholarly publications.
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KEYWORDS
Spectrographs

Cameras

Spectroscopy

Imaging systems

Astronomical imaging

CCD cameras

Spectral resolution

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