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Physical properties and transmission spectrum of the WASP-80 planetary system from multi-colour photometry

文献类型:期刊论文

作者Mancini, L1; Southworth, J2; Ciceri, S1; Dominik, M3; Henning, T1; Jorgensen, UG4,5; Lanza, AF6; Rabus, M1,7; Snodgrass, C8; Vilela, C2
刊名ASTRONOMY & ASTROPHYSICS
出版日期2014-02
卷号562
ISSN号0004-6361
关键词planetary systems stars: fundamental parameters stars: individual: WASP-80 techniques: photometric
通讯作者Mancini, L (reprint author), Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany.
产权排序第十五完成单位
英文摘要WASP-80 is one of only two systems known to contain a hot Jupiter which transits its M-dwarf host star. We present eight light curves of one transit event, obtained simultaneously using two defocussed telescopes. These data were taken through the Bessell I, Sloan g' r' i' z' and near-infrared JHK passbands. We use our data to search for opacity-induced changes in the planetary radius, but find that all values agree with each other. Our data are therefore consistent with a flat transmission spectrum to within the observational uncertainties. We also measure an activity index of the host star of log R-HK' = -4.495, meaning that WASP-80A shows strong chromospheric activity. The non-detection of starspots implies that, if they exist, they must be small and symmetrically distributed on the stellar surface. We model all available optical transit light curves and obtain improved physical properties and orbital ephemerides for the system.
学科主题Astronomy & Astrophysics
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]TRANSITING EXTRASOLAR PLANETS ; EARTH GJ 1214B ; STELLAR EVOLUTION DATABASE ; HUBBLE-SPACE-TELESCOPE ; HOT JUPITERS ; TIDAL-EVOLUTION ; COOL STARS ; ATMOSPHERE ; MODELS ; MASS
收录类别SCI ; EI
原文出处http://www.aanda.org/articles/aa/abs/2014/02/aa23265-13/aa23265-13.html
语种英语
WOS记录号WOS:000332161800155
源URL[http://ir.ynao.ac.cn/handle/114a53/6802]  
专题云南天文台_系外行星研究组
云南天文台_中国科学院天体结构与演化重点实验室
作者单位1.Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
2.Astrophysics Group, Keele University, Keele, ST5 5BG, UK
3.SUPA, University of St Andrews, School of Physics & Astronomy, North Haugh, St Andrews KY16 9SS, UK
4.Niels Bohr Institute, University of Copenhagen, Juliane Maries vej 30, 2100 Copenhagen Ø, Denmark
5.Centre for Star and Planet Formation, Geological Museum, Øster Voldgade 5-7, 1350 Copenhagen, Denmark
6.INAF-Osservatorio Astrofisico di Catania, via S.Sofia 78, 95123 Catania, Italy
7.Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 7820436 Macul, Santiago, Chile
8.Max-Planck-Institute for Solar System Research, Max-Planck Str. 2, 37191 Katlenburg-Lindau, Germany
9.Qatar Foundation, PO Box 5825, Doha, Qatar
10.Dipartimento di Fisica “E.R. Caianiello”, University of Salerno, via Giovanni Paolo II, 84084 Fisciano, Italy
推荐引用方式
GB/T 7714
Mancini, L,Southworth, J,Ciceri, S,et al. Physical properties and transmission spectrum of the WASP-80 planetary system from multi-colour photometry[J]. ASTRONOMY & ASTROPHYSICS,2014,562.
APA Mancini, L.,Southworth, J.,Ciceri, S.,Dominik, M.,Henning, T.,...&Wertz, O.(2014).Physical properties and transmission spectrum of the WASP-80 planetary system from multi-colour photometry.ASTRONOMY & ASTROPHYSICS,562.
MLA Mancini, L,et al."Physical properties and transmission spectrum of the WASP-80 planetary system from multi-colour photometry".ASTRONOMY & ASTROPHYSICS 562(2014).

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来源:云南天文台

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