中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing

文献类型:期刊论文

作者Li, S. -S.2,3; Zang, W.4,5; Udalski, A.6; Shvartzvald, Y.7; Huber, D.8; Lee, C. -U.9,10; Sumi, T.11; Gould, A.9,12,13; Mao, S.2,4,5; Fouque, P.14,15
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2019-09-01
卷号488期号:3页码:3308-3323
ISSN号0035-8711
关键词asteroseismology gravitational lensing: micro stars: fundamental parameters stars: oscillations
DOI10.1093/mnras/stz1873
英文摘要We present the analysis of the event OGLE-2017-B1,G-1186 from the 2017.Spitzer microlensing campaign. This is a remarkable microlensing event because its source is photometrically bright and variable, which makes it possible to perform an asteroseismic analysis using ground-based data. We find that the source star is an oscillating red giant with average time scale of similar to 9 d. The asteroseismic analysis also provides us source properties including the source angular size (similar to 27 as) and distance (similar to 11.5 kpc), which are essential for inferring the properties of the lens. When fitting the light curve, we test the feasibility of Gaussian processes (GPs) in handling the correlated noise caused by the variable source. We find that the parameters from the GP model are generally more loosely constrained than those from the traditional chi(2) minimization method. We note that this event is the first microlensing system for which asteroseismology and GPs have been used to account for the variable source. With both finite-source effect and microlens parallax measured, we find that the lens is likely a similar to 0,045 M-circle dot brown dwarf at distance similar to 9.0 kpc, or a similar to 0.073 M-circle dot ultracool dwarf at distance similar to 9.8 kpc. Combining the estimated lens properties with a Bayesian analysis using a Galactic model, we find a similar to 35 per cent probability for the lens to be a bulge object and similar to 65 per cent to be a background disc object.
WOS关键词SURFACE BRIGHTNESS RELATIONS ; STELLAR OSCILLATIONS ; PLANET PHOTOMETRY ; ANGULAR SIZES ; DWARF STARS ; SYSTEMS ; SUBGIANTS ; DISTANCES ; STANDARD ; PROGRAM
资助项目National Science Foundation of China[11821303] ; National Science Foundation of China[11761131004] ; National Science Centre, Poland[MAESTRO 2014/14/A/ST9/00121] ; National Science Foundation[AST-1717000] ; JSPS KAKENHI[JSPS24253004] ; JSPS KAKENHI[JSPS26247023] ; JSPS KAKENHI[JSPS23340064] ; JSPS KAKENHI[JSPS15H00781] ; JSPS KAKENHI[JP16H06287] ; JSPS KAKENHI[JP17H02871] ; US NSF[AST-1516842] ; JPL grant[1500811] ; Canada-France-Hawaii Telescope (CFHT)[11573003] ; National Science Foundation of China (NSFC)[11573003] ; National Research Foundation of Korea[2017R1A4A1015178] ; DFG[SPP 1992] ; DFG[WA 1047/11-1] ; National Funds through FCT -Foundation for Science and Technology[UID/Multi/00611/2013] ; FEDER -European Regional Development Fund[POCI-01-0145-FEDER-006922] ; Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund ; University of Tasmania through the UTAS Foundation ; CNES ; Australian Research Council's LIEF funding scheme[LE110100055] ; National Aeronautics and Space Administration ; National Science Foundation ; ANR COLD-WORLDS[ANR-18-CE31-0002]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:000485158400026
资助机构National Science Foundation of China ; National Science Foundation of China ; National Science Centre, Poland ; National Science Centre, Poland ; National Science Foundation ; National Science Foundation ; JSPS KAKENHI ; JSPS KAKENHI ; US NSF ; US NSF ; JPL grant ; JPL grant ; Canada-France-Hawaii Telescope (CFHT) ; Canada-France-Hawaii Telescope (CFHT) ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; National Research Foundation of Korea ; National Research Foundation of Korea ; DFG ; DFG ; National Funds through FCT -Foundation for Science and Technology ; National Funds through FCT -Foundation for Science and Technology ; FEDER -European Regional Development Fund ; FEDER -European Regional Development Fund ; Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund ; Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund ; University of Tasmania through the UTAS Foundation ; University of Tasmania through the UTAS Foundation ; CNES ; CNES ; Australian Research Council's LIEF funding scheme ; Australian Research Council's LIEF funding scheme ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; ANR COLD-WORLDS ; ANR COLD-WORLDS ; National Science Foundation of China ; National Science Foundation of China ; National Science Centre, Poland ; National Science Centre, Poland ; National Science Foundation ; National Science Foundation ; JSPS KAKENHI ; JSPS KAKENHI ; US NSF ; US NSF ; JPL grant ; JPL grant ; Canada-France-Hawaii Telescope (CFHT) ; Canada-France-Hawaii Telescope (CFHT) ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; National Research Foundation of Korea ; National Research Foundation of Korea ; DFG ; DFG ; National Funds through FCT -Foundation for Science and Technology ; National Funds through FCT -Foundation for Science and Technology ; FEDER -European Regional Development Fund ; FEDER -European Regional Development Fund ; Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund ; Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund ; University of Tasmania through the UTAS Foundation ; University of Tasmania through the UTAS Foundation ; CNES ; CNES ; Australian Research Council's LIEF funding scheme ; Australian Research Council's LIEF funding scheme ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; ANR COLD-WORLDS ; ANR COLD-WORLDS ; National Science Foundation of China ; National Science Foundation of China ; National Science Centre, Poland ; National Science Centre, Poland ; National Science Foundation ; National Science Foundation ; JSPS KAKENHI ; JSPS KAKENHI ; US NSF ; US NSF ; JPL grant ; JPL grant ; Canada-France-Hawaii Telescope (CFHT) ; Canada-France-Hawaii Telescope (CFHT) ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; National Research Foundation of Korea ; National Research Foundation of Korea ; DFG ; DFG ; National Funds through FCT -Foundation for Science and Technology ; National Funds through FCT -Foundation for Science and Technology ; FEDER -European Regional Development Fund ; FEDER -European Regional Development Fund ; Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund ; Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund ; University of Tasmania through the UTAS Foundation ; University of Tasmania through the UTAS Foundation ; CNES ; CNES ; Australian Research Council's LIEF funding scheme ; Australian Research Council's LIEF funding scheme ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; ANR COLD-WORLDS ; ANR COLD-WORLDS ; National Science Foundation of China ; National Science Foundation of China ; National Science Centre, Poland ; National Science Centre, Poland ; National Science Foundation ; National Science Foundation ; JSPS KAKENHI ; JSPS KAKENHI ; US NSF ; US NSF ; JPL grant ; JPL grant ; Canada-France-Hawaii Telescope (CFHT) ; Canada-France-Hawaii Telescope (CFHT) ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; National Research Foundation of Korea ; National Research Foundation of Korea ; DFG ; DFG ; National Funds through FCT -Foundation for Science and Technology ; National Funds through FCT -Foundation for Science and Technology ; FEDER -European Regional Development Fund ; FEDER -European Regional Development Fund ; Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund ; Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund ; University of Tasmania through the UTAS Foundation ; University of Tasmania through the UTAS Foundation ; CNES ; CNES ; Australian Research Council's LIEF funding scheme ; Australian Research Council's LIEF funding scheme ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; ANR COLD-WORLDS ; ANR COLD-WORLDS
源URL[http://ir.bao.ac.cn/handle/114a11/27707]  
专题中国科学院国家天文台
通讯作者Li, S. -S.
作者单位1.Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
3.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
4.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
5.Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100084, Peoples R China
6.Univ Warsaw Observ, Al Ujazdowskie 4, PL-00478 Warsaw, Poland
7.CALTECH, IPAC, Mail Code 100-22,1200 E Calif Blvd, Pasadena, CA 91125 USA
8.Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA
9.Korea Astron & Space Sci Inst, Daejon 34055, South Korea
10.Univ Sci & Technol Korea UST, Astron & Space Sci Major, 217 Gajeong Ro, Daejeon 34113, South Korea
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Li, S. -S.,Zang, W.,Udalski, A.,et al. OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,488(3):3308-3323.
APA Li, S. -S..,Zang, W..,Udalski, A..,Shvartzvald, Y..,Huber, D..,...&Hill, K..(2019).OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,488(3),3308-3323.
MLA Li, S. -S.,et al."OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 488.3(2019):3308-3323.

入库方式: OAI收割

来源:国家天文台

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