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High-precision photometry by telescope defocussing - VI. WASP-24, WASP-25 and WASP-26
Southworth, J1; Hinse, TC2; Burgdorf, M3; Novati, SC4,5; Dominik, M6; Galianni, P6; Gerner, T7; Giannini, E7; Gu SH(顾盛宏)8,9; Hundertmark, M6
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2014-10-11
卷号444期号:1页码:776-789
关键词stars: fundamental parameters planetary systems stars: individual: WASP-24 stars: individual: WASP-25 stars: individual: WASP-26
ISSN号0035-8711
通讯作者Southworth, J (reprint author), Keele Univ, Astrophys Grp, Keele ST5 5BG, Staffs, England.
产权排序第八完成单位
英文摘要We present time series photometric observations of 13 transits in the planetary systems WASP-24, WASP-25 and WASP-26. All three systems have orbital obliquity measurements, WASP-24 andWASP-26 have been observed with Spitzer, andWASP-25 was previously comparatively neglected. Our light curves were obtained using the telescope-defocussing method and have scatters of 0.5-1.2 mmag relative to their best-fitting geometric models. We use these data to measure the physical properties and orbital ephemerides of the systems to high precision, finding that our improved measurements are in good agreement with previous studies. High-resolution Lucky Imaging observations of all three targets show no evidence for faint stars close enough to contaminate our photometry. We confirm the eclipsing nature of the star closest to WASP-24 and present the detection of a detached eclipsing binary within 4.25 arcmin of WASP-26.
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 ; STELLAR EVOLUTION DATABASE ; PHYSICAL-PROPERTIES ; GIANT PLANETS ; ECLIPSING BINARIES ; STARS ; SYSTEM ; PARAMETERS ; RADII ; EXOPLANETS
收录类别SCI
原文出处http://mnras.oxfordjournals.org/content/444/1/776
语种英语
WOS记录号WOS:000342925100059
内容类型期刊论文
源URL[http://ir.ynao.ac.cn/handle/114a53/6798]  
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.Astrophysics Group, Keele University, Staffordshire ST5 5BG, UK
2.Korea Astronomy and Space Science Institute, Daejeon 305-348, Republic of Korea
3.HE Space Operations GmbH, Flughafenallee 24, D-28199 Bremen, Germany
4.Dipartimento di Fisica ‘E.R. Caianiello’, Università di Salerno, Via Giovanni Paolo II 132, I-84084 Fisciano (SA), Italy
5.Istituto Internazionale per gli Alti Studi Scientifici (IIASS), I-84019 Vietri Sul Mare (SA), Italy
6.SUPA, University of St Andrews, School of Physics and Astronomy, North Haugh, St Andrews KY16 9SS, UK
7.Astronomisches Rechen-Institut, Zentrum für Astronomie, Universität Heidelberg, Mönchhofstraße 12-14, D-69120 Heidelberg, Germany
8.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
9.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
10.Niels Bohr Institute & Centre for Star and Planet Formation, University of Copenhagen, Juliane Maries vej 30, DK-2100 Copenhagen Ø, Denmark
推荐引用方式
GB/T 7714
Southworth, J,Hinse, TC,Burgdorf, M,et al. High-precision photometry by telescope defocussing - VI. WASP-24, WASP-25 and WASP-26[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2014,444(1):776-789.
APA Southworth, J.,Hinse, TC.,Burgdorf, M.,Novati, SC.,Dominik, M.,...&Vilela, C.(2014).High-precision photometry by telescope defocussing - VI. WASP-24, WASP-25 and WASP-26.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,444(1),776-789.
MLA Southworth, J,et al."High-precision photometry by telescope defocussing - VI. WASP-24, WASP-25 and WASP-26".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 444.1(2014):776-789.
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