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题名: The bright star survey telescope for the planetary transit survey in Antarctica
作者: Tian, Qiguo1; Jiang, Peng1, 2; Du, Fujia3; Wang, Jian4; Li, Zhengyang3; Li, Xiaoyan3; Zhang, Zhiyong3; Lu, Haiping3; Yuan, Xiangyan3; Liu, Huigen2, 5; Zhang, Hui2, 5; Sun, Luming1, 6; Chang, Liang7, 8; Wang, Jianguo7, 8; Zhang, Shaohua1; Ji, Tuo1; Shi, Xiheng1; Chen, Jie4; Zhang, Guangyu4; Jia, Minghao4; Liu, Jiajing4; Zhou, Junyan1, 2, 6; Pan, Xiang1, 6; Dong, Shucheng4; Jiang, Fengxin4; Zhang, Hongfei4; Zhou, Jilin5; Wang LiFan(王力帆)9; Zhou, Hongyan1, 6
刊名: SCIENCE BULLETIN
出版日期: 2016-03-01
卷号: 61, 期号:5, 页码:383-390
关键词: Instrumentation ; Exoplanet ; Photometry ; Antarctic Site
DOI: 10.1007/s11434-016-1015-0
文章类型: Article
英文摘要: Transiting extrasolar planets (exoplanets), especially those orbiting bright stars, are desired for study of the diversity of planetary compositions, internal structures and atmospheres beyond our solar system. Dome A at Antarctica is a promising site for planetary transit surveys, where the continuous darkness and the large clear-sky fraction in the winter months greatly enhance the detection efficiency. The Chinese Small Telescope ARray and the Antarctic Survey Telescopes are the first facilities that have been operated at Dome A for use in exoplanet surveys. To increase the sky coverage, a low-temperature-resistant wide-field robotic telescope, named the bright star survey telescope (BSST), has been developed to join the ongoing planetary transit survey in Antarctica. The BSST has an aperture size of 300 mm and is equipped with a large-frame 4k x 4k CCD camera to receive starlight from a 3.degrees 4 x 3.degrees 4 field of view. The BSST was operated at Lijiang observatory in April and May 2015 for a test run. Photometric precision of 3.5 mmag was achieved for stars with V similar to 11 mag using 75 s exposures. The transiting events of two Jupiter-size exoplanets, HAT-P-3b and HAT-P-12b, were observed on May 10 and May 20, 2015, respectively.
WOS标题词: Science & Technology
类目[WOS]: Multidisciplinary Sciences
研究领域[WOS]: Science & Technology - Other Topics
关键词[WOS]: DIGITAL SKY SURVEY ; K-DWARF ; DOME-C ; PHOTOMETRY ; MASS ; SCINTILLATION ; ATMOSPHERE ; COMPANION
收录类别: SCI
项目资助者: Astronomical Project for the Chinese Antarctic Inland Station, SOC Program(CHINARE201202-03 ; National Basic Research Program of China(2013CB834905 ; National Natural Science Foundation of China(11503023 ; Natural Science Foundation of Shanghai(14ZR1444100 ; Polar Science Innovation Fund for Young Scientists of Polar Research Institute of China(CX20130201) ; CHINARE2013-02-03 ; 2015CB857005) ; 11233002 ; 15ZR1444200) ; CHINARE2014-02-03 ; 11203022 ; CHINARE2015-02-03) ; 11473025 ; 11421303 ; 11033007 ; 11573024 ; 11503022)
语种: 英语
WOS记录号: WOS:000371276900007
Citation statistics:
内容类型: 期刊论文
URI标识: http://libir.pmo.ac.cn/handle/332002/16163
Appears in Collections:南极天文中心_期刊论文

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作者单位: 1.Polar Res Inst China, Shanghai 200136, Peoples R China
2.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China
3.Chinese Acad Sci, Natl Astron Observ, Nanjing Inst Astron Opt & Technol, Nanjing 210042, Jiangsu, Peoples R China
4.Univ Sci & Technol China, Dept Modern Phys, State Key Lab Technol Particle Detect & Elect, Hefei 230026, Peoples R China
5.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210093, Jiangsu, Peoples R China
6.Univ Sci & Technol China, Chinese Acad Sci, Dept Astron, Key Lab Res Galaxies & Cosmol, Hefei 230026, Peoples R China
7.Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China
8.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Peoples R China
9.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
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