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Performance and sensitivity of Low Resolution Spectrographs for LAMOST
Yonghui Hou; Yongtian Zhu; Zhongwen Hu; Lei Wang; Jianing Wang
2010-07-14
Source PublicationGround-based and Airborne Instrumentation for Astronomy III
Volume7735
Issue7735
PagesVol.7735 0C-1-9
Conference Date2010-6-27
Conference PlaceSan Diego, California, USA
Funding OrganizationThe International Society for Optical Engineering
PublisherSPIE
Abstract
The 16 low resolution spectrographs (LRS) have been successfully commissioned for the LAMOST. The LRS design employs a dual-beamed and bench-mounted, with large-beamed, fast Schmidt cameras and Volume Phase Holographic (VPH) transmission gratings. The design wavelength range is 370-900nm, at resolutions of R=1000and R=10000. Each spectrograph is fed by 250 fibers with 320 micron in diameter (corresponding 3.3 arcsec), composed of one F/4 Schmidt collimator, a dichroic beam-splitter, four VPH gratings, articulating Schmidt cameras that are optimized at blue band
(370-590 nm) and red band (570-900 nm), and field lens near the focal plane service as the vacuum window of CCD detector cryogenic head. In this paper, we present the testing result of the LRS on the image quality, spectra resolution, efficiency and observing spectra.
KeywordSpectrograph Multi-fibers Spectra Survey.
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/114a32/614
Collection会议论文
Recommended Citation
GB/T 7714
Yonghui Hou,Yongtian Zhu,Zhongwen Hu,et al. Performance and sensitivity of Low Resolution Spectrographs for LAMOST[C]:SPIE,2010:Vol.7735 0C-1-9.
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