The Xinglong 2.16-m Telescope: Current Instruments and Scientific Projects
文献类型:期刊论文
作者 | Fan, Zhou1; Wang, Huijuan1; Jiang, Xiaojun1; Wu, Hong1; Li, Hongbin1; Huang, Yang2; Xu, Dawei3; Hu, Zhongwen4; Zhu, Yinan1; Wang, Jianfeng1 |
刊名 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC |
出版日期 | 2016-11-01 |
卷号 | 128期号:969 |
关键词 | instrumentation: miscellaneous instrumentation: photometers instrumentation: spectrographs telescopes |
英文摘要 | The Xinglong 2.16-m reflector is the first 2-m class astronomical telescope in China. It was jointly designed and built by the Nanjing Astronomical Instruments Factory (NAIF), Beijing Astronomical Observatory (now National Astronomical Observatories, Chinese Academy of Sciences, NAOC), and Institute of Automation, Chinese Academy of Sciences in 1989. It is a Ritchey-Chretien (R-C) reflector on an English equatorial mount and the effective aperture is 2.16 m. It had been the largest optical telescope in China for similar to 18 years until the Guoshoujing Telescope (also called Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) and the Lijiang 2.4-m telescope were built. At present, there are three main instruments on the Cassegrain focus available: the Beijing Faint Object Spectrograph and Camera (BFOSC) for direct imaging and low-resolution (R similar to 500-2000) spectroscopy, the spectrograph made by Optomechanics Research Inc. (OMR) for low-resolution spectroscopy (the spectral resolutions are similar to those of BFOSC) and the fiber-fed High Resolution Spectrograph (HRS; R similar to 30,000-65,000). The telescope is widely open to astronomers all over China as well as international astronomical observers. Each year there are more than 40 ongoing observing projects, including 6-8 key projects. Recently, some new techniques and instruments (e.g., astro-frequency comb calibration system, polarimeter, and adaptive optics) have been or will be tested on the telescope to extend its observing abilities. |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | BLUE COMPACT GALAXIES ; OPTICAL/NEAR-INFRARED COLORS ; SUBSTELLAR COMPANION ; SYSTEM ; SPECTROGRAPH ; METALLICITY ; QUASARS |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000387113900011 |
源URL | [http://ir.bao.ac.cn/handle/114a11/6856] |
专题 | 国家天文台_光学天文研究部 |
作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, 20A Datun Rd, Beijing 100012, Peoples R China 2.Peking Univ, Dept Astron, Beijing 100871, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, Key Lab Space Astron & Technol, 20A Datun Rd, Beijing 100012, Peoples R China 4.Chinese Acad Sci, Natl Astron Observ, Nanjing Inst Astron Opt & Technol, 188 Bancang St, Nanjing 210042, Jiangsu, Peoples R China 5.Max Planck Inst Radioastron, Huegel 69, D-53121 Bonn, Germany |
推荐引用方式 GB/T 7714 | Fan, Zhou,Wang, Huijuan,Jiang, Xiaojun,et al. The Xinglong 2.16-m Telescope: Current Instruments and Scientific Projects[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,2016,128(969). |
APA | Fan, Zhou.,Wang, Huijuan.,Jiang, Xiaojun.,Wu, Hong.,Li, Hongbin.,...&Zhu,Yinan.(2016).The Xinglong 2.16-m Telescope: Current Instruments and Scientific Projects.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,128(969). |
MLA | Fan, Zhou,et al."The Xinglong 2.16-m Telescope: Current Instruments and Scientific Projects".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 128.969(2016). |
入库方式: OAI收割
来源:国家天文台
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