The LAMOST middle resolution spectrograph
文献类型：会议论文
| 作者 | 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
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| 出版日期 | 2018-07-06 |
| 会议名称 | SPIE Ground-based and Airborne Instrumentation for Astronomy VII（Vol.10702） |
| 会议日期 | 2018-6-10 |
| 会议地点 | Austin, Texas, United States |
| 关键词 | Spectrograph Astronomical Instrumentation Optical Design LAMOST |
| 英文摘要 |
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). |
| 会议录 | Ground-based and Airborne Instrumentation for Astronomy VII
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| 学科主题 | 天文技术与方法 |
| 语种 | 英语 |
| 源URL | [http://ir.niaot.ac.cn/handle/114a32/1561]  |
| 专题 | 会议论文 |
| 作者单位 | 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 |
| 推荐引用方式 GB/T 7714 | 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. |
入库方式： OAI收割
来源：南京天文光学技术研究所
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