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 |
关键词 | planetary systems stars: fundamental parameters stars: individual: WASP-80 techniques: photometric |
ISSN号 | 0004-6361 |
产权排序 | 第十五完成单位 |
通讯作者 | Mancini, L (reprint author), Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany. |
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. |
WOS标题词 | Science & Technology ; Physical Sciences |
学科主题 | Astronomy & Astrophysics |
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). |
入库方式: OAI收割
来源:云南天文台
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。