TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS
文献类型:期刊论文
作者 | Davis,Allen B.5; Wang,Songhu5; Jones,Matias6,7; Eastman,Jason D.8; Günther,Maximilian N.9; Stassun,Keivan G.10,11; Addison,Brett C.12; Collins,Karen A.8; Quinn,Samuel N.8; Latham,David W.8 |
刊名 | The Astronomical Journal
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出版日期 | 2020-10-29 |
卷号 | 160期号:5 |
关键词 | Exoplanet astronomy Exoplanet detection methods Radial velocity Transit photometry Extrasolar gas giants Hot Jupiters |
ISSN号 | 0004-6256 |
DOI | 10.3847/1538-3881/aba49d |
英文摘要 | Abstract We report the discovery and confirmation of two new hot Jupiters discovered by the Transiting Exoplanet Survey Satellite (TESS): TOI 564 b and TOI 905 b. The transits of these two planets were initially observed by TESS with orbital periods of 1.651 and 3.739 days, respectively. We conducted follow-up observations of each system from the ground, including photometry in multiple filters, speckle interferometry, and radial velocity measurements. For TOI 564 b, our global fitting revealed a classical hot Jupiter with a mass of MJ and a radius of RJ. Also a classical hot Jupiter, TOI 905 b has a mass of MJ and radius of RJ. Both planets orbit Sun-like, moderately bright, mid-G dwarf stars with V?~?11. While TOI 905 b fully transits its star, we found that TOI 564 b has a very high transit impact parameter of , making it one of only ~20 known systems to exhibit a grazing transit and one of the brightest host stars among them. Therefore, TOI 564 b is one of the most attractive systems to search for additional nontransiting, smaller planets by exploiting the sensitivity of grazing transits to small changes in inclination and transit duration over a timescale of several years. |
语种 | 英语 |
WOS记录号 | IOP:0004-6256-160-5-ABA49D |
出版者 | The American Astronomical Society |
源URL | [http://ir.bao.ac.cn/handle/114a11/61567] ![]() |
专题 | 中国科学院国家天文台 |
通讯作者 | Davis,Allen B. |
作者单位 | 1.Brierfield Observatory, New South Wales, Australia 2.The Maury Lewin Astronomical Observatory, Glendora, CA 91741, USA 3.Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA 4.Department of Physics and Astronomy, The University of North Carolina at Chapel Hill, Chapel Hill, NC 27599, USA 5.Department of Astronomy, Yale University, 52 Hillhouse Avenue, New Haven, CT 06511, USA; allen.b.davis@yale.edu 6.European Southern Observatory, Alonso de Córdova 3107, Vitacura, Casilla 19001, Santiago, Chile 7.Instituto de Astronomía, Universidad Católica del Norte, Angamos 0610, 1270709, Antofagasta, Chile 8.Center for Astrophysics ∣ Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA 9.Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA 10.Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235, USA |
推荐引用方式 GB/T 7714 | Davis,Allen B.,Wang,Songhu,Jones,Matias,et al. TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS[J]. The Astronomical Journal,2020,160(5). |
APA | Davis,Allen B..,Wang,Songhu.,Jones,Matias.,Eastman,Jason D..,Günther,Maximilian N..,...&Fischer,Debra A..(2020).TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS.The Astronomical Journal,160(5). |
MLA | Davis,Allen B.,et al."TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS".The Astronomical Journal 160.5(2020). |
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来源:国家天文台
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