Paper
24 September 2012 The LAMOST low resolution spectrograph stability performance
YongHui Hou, Lei Wang, Zhongwen Hu, Jianing Wang, Zhen Tang, Mingda Jiang, Yongtian Zhu
Author Affiliations +
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.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
YongHui Hou, Lei Wang, Zhongwen Hu, Jianing Wang, Zhen Tang, Mingda Jiang, and Yongtian Zhu "The LAMOST low resolution spectrograph stability performance", Proc. SPIE 8446, Ground-based and Airborne Instrumentation for Astronomy IV, 844660 (24 September 2012); https://doi.org/10.1117/12.925640
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Spectrographs

Charge-coupled devices

Astronomical imaging

Telescopes

Galactic astronomy

Spectroscopy

Liquids

RELATED CONTENT


Back to Top