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The bright star survey telescope for the planetary transit survey in Antarctica
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 L(常亮)7,8; Wang JG(王建国)7,8; Zhang, Shaohua1; Ji, Tuo1; Shi, Xiheng1; Chen, Jie4; Zhang, Guangyu4; Jia, Minghao4; Liu, Jiajing4; Zhou, Junyan1,6; Pan, Xiang1,6; Dong, Shucheng4; Jiang, Fengxin4; Zhang, Hongfei4; Zhou, Jilin2,5; Wang, Lifan9; Zhou, Hongyan1,6; Jiang, P (reprint author), Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China.
发表期刊SCIENCE BULLETIN
2016-03-01
卷号61期号:5页码:383-390
DOI10.1007/s11434-016-1015-0
产权排序第7完成单位
收录类别SCI ; EI
关键词Instrumentation Exoplanet Photometry Antarctic Site
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.
项目资助者Astronomical Project for the Chinese Antarctic Inland Station, SOC Program(CHINARE201202-03, CHINARE2013-02-03, CHINARE2014-02-03, CHINARE2015-02-03) ; National Basic Research Program of China(2013CB834905, 2015CB857005) ; National Natural Science Foundation of China(11503023, 11233002, 11203022, 11473025, 11421303, 11033007, 11573024, 11503022) ; Natural Science Foundation of Shanghai(14ZR1444100, 15ZR1444200) ; Polar Science Innovation Fund for Young Scientists of Polar Research Institute of China(CX20130201)
语种英语
学科领域Science & Technology - Other Topics
文章类型Article
ISSN2095-9273
URL查看原文
WOS记录号WOS:000371276900007
WOS研究方向Science & Technology - Other Topics
WOS类目Multidisciplinary Sciences
关键词[WOS]DIGITAL SKY SURVEY ; K-DWARF ; DOME-C ; PHOTOMETRY ; MASS ; SCINTILLATION ; ATMOSPHERE ; COMPANION
引用统计
被引频次:7[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9348
专题丽江天文观测站(南方基地)
中国科学院天体结构与演化重点实验室
通讯作者Jiang, P (reprint author), Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China.
作者单位1.Polar Research Institute of China, Shanghai, 200136, China
2.School of Astronomy and Space Science, Nanjing University, Nanjing, 210093, China
3.National Astronomical Observatories/Nanjing Institute of Astronomical Optics and Technology, Chinese Academy of Sciences, Nanjing, 210042, China
4.State Key Laboratory of Technologies of Particle Detection and Electronics, Department of Modern Physics, University of Science and Technology of China, Hefei, 230026, China
5.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing, 210093, China
6.Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Chinese Academy of Sciences, Hefei, 230026, China
7.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, China
8.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, 650011, China
9.Purple Mountain Observatory, Chinese Academy of Science, Nanjing, 210008, China
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Tian, Qiguo,Jiang, Peng,Du, Fujia,et al. The bright star survey telescope for the planetary transit survey in Antarctica[J]. SCIENCE BULLETIN,2016,61(5):383-390.
APA Tian, Qiguo.,Jiang, Peng.,Du, Fujia.,Wang, Jian.,Li, Zhengyang.,...&Jiang, P .(2016).The bright star survey telescope for the planetary transit survey in Antarctica.SCIENCE BULLETIN,61(5),383-390.
MLA Tian, Qiguo,et al."The bright star survey telescope for the planetary transit survey in Antarctica".SCIENCE BULLETIN 61.5(2016):383-390.
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