中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Physical properties of the planetary systemsWASP-45 and WASP-46 from simultaneous multiband photometry

文献类型:期刊论文

作者Ciceri, S.1; Mancini, L.1,2; Southworth, J.3; Lendl, M.4,5; Tregloan-Reed, J.3,6; Brahm, R.7,8; Chen, G.9,10; D'Ago, G.11,12,13; Dominik, M.14; Jaimes, R. Figuera13,15
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2016-02-11
卷号456期号:1页码:990-1002
关键词planets and satellites: fundamental parameters stars: fundamental parameters stars: individual: WASP-45 stars: individual: WASP-46
英文摘要Accurate measurements of the physical characteristics of a large number of exoplanets are useful to strongly constrain theoretical models of planet formation and evolution, which lead to the large variety of exoplanets and planetary-system configurations that have been observed. We present a study of the planetary systems WASP-45 and WASP-46, both composed of a main-sequence star and a close-in hot Jupiter, based on 29 new high-quality light curves of transits events. In particular, one transit of WASP-45 b and four of WASP-46 b were simultaneously observed in four optical filters, while one transit of WASP-46 b was observed with the NTT obtaining a precision of 0.30 mmag with a cadence of roughly 3 min. We also obtained five new spectra of WASP-45 with the FEROS spectrograph. We improved by a factor of 4 the measurement of the radius of the planet WASP-45 b, and found that WASP-46 b is slightly less massive and smaller than previously reported. Both planets now have a more accurate measurement of the density (0.959 +/- 0.077 rho Jup instead of 0.64 +/- 0.30 rho Jup for WASP-45 b, and 1.103 +/- 0.052 rho Jup instead of 0.94 +/- 0.11 rho Jup for WASP-46 b). We tentatively detected radius variations with wavelength for both planets, in particular in the case of WASP-45 b we found a slightly larger absorption in the redder bands than in the bluer ones. No hints for the presence of an additional planetary companion in the two systems were found either from the photometric or radial velocity measurements.
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 ; STELLAR EVOLUTION DATABASE ; HIGH-PRECISION PHOTOMETRY ; LIMB-DARKENING LAW ; LIGHT-CURVE ; TRANSMISSION SPECTRA ; ATMOSPHERE MODELS ; SURFACE GRAVITIES ; LOW-MASS ; TELESCOPE
收录类别SCI
语种英语
WOS记录号WOS:000368010000107
源URL[http://libir.pmo.ac.cn/handle/332002/16109]  
专题紫金山天文台_行星科学与深空探测实验室
作者单位1.Max Planck Inst Astron, D-69117 Heidelberg, Germany
2.Osserv Astron Torino, INAF, I-10025 Pino Torinese, Italy
3.Keele Univ, Astrophys Grp, Keele ST5 5BG, Staffs, England
4.Austrian Acad Sci, Space Res Inst, A-8042 Graz, Austria
5.Univ Geneva, Observ Geneva, CH-1290 Sauverny, Switzerland
6.NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
7.Pontificia Univ Catolica Chile, Inst Astrofis, Santiago 7820436, Chile
8.Millennium Inst Astrophys, Santiago 7820436, Chile
9.Chinese Acad Sci, Purple Mt Observ, Key Lab Planetary Sci, Nanjing 210008, Jiangsu, Peoples R China
10.Inst Astrofis Canarias, E-38205 Tenerife, Spain
推荐引用方式
GB/T 7714
Ciceri, S.,Mancini, L.,Southworth, J.,et al. Physical properties of the planetary systemsWASP-45 and WASP-46 from simultaneous multiband photometry[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2016,456(1):990-1002.
APA Ciceri, S..,Mancini, L..,Southworth, J..,Lendl, M..,Tregloan-Reed, J..,...&Wertz, O..(2016).Physical properties of the planetary systemsWASP-45 and WASP-46 from simultaneous multiband photometry.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,456(1),990-1002.
MLA Ciceri, S.,et al."Physical properties of the planetary systemsWASP-45 and WASP-46 from simultaneous multiband photometry".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 456.1(2016):990-1002.

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