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The LAMOST low resolution spectrograph Stability Performance
Yonghui Hou; Lei Wang; Zhongwen Hu; Jianing Wang; Zhen Tang; Mingda Jiang; Yongtian Zhu
2012-09-24
Source PublicationGround-based and Airborne Instrumentation for Astronomy IV
Volume8446
Issue8446
PagesVol.8446 60-1-6
Conference Date2012-7-1
Conference PlaceAmsterdam, Netherlands
Funding OrganizationThe International Society for Optical Engineering
PublisherSPIE
Abstract
One of the Large Sky Area Multi-Object Spectroscopic Telescope (LAMOST) scientific requirements require the ability of the low resolution spectrograph(LRS) to measure velocities to a accuracy of 4km/s over the entire 5 degree field in 2 hours objects observation. This requirement results in the specification of image movement less than 0.6μm/hours (0.05pixl/hours corresponding to the science detector).There are 16 spectrographs for LAMOST telescope, so we expect the design aspects of the instrument directed towards achieving the stability goal. In this paper we present the last design aspects of the instrument which enable meeting the 4km/s requirement, and the recent test results of the LRS’s Stability Performance. The test results show that the stability performance of LAMOST-LRS can meet the the stability goal, the image shift along the direction of dispersion is not influenced by the external factors, and the image shift along vertical dispersion direction meet the technical requirements when the environmental temperature of the spectrograph room is in control.
KeywordAstronomical Instrumentation Lamost Spectrograph Stability
Subject Area郭守敬望远镜(lamost) ; 天文光谱仪
Document Type会议论文
Identifierhttp://ir.niaot.ac.cn/handle/114a32/682
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
Recommended Citation
GB/T 7714
Yonghui Hou,Lei Wang,Zhongwen Hu,et al. The LAMOST low resolution spectrograph Stability Performance[C]:SPIE,2012:Vol.8446 60-1-6.
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