中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Confirmation of a Sub-Saturn-size Transiting Exoplanet Orbiting a G Dwarf: TOI-1194 b and a Very Low Mass Companion Star: TOI-1251 B from TESS

文献类型:期刊论文

作者Wang, Jia-Qi18,19; Jiang, Xiao-Jun18,19; Zheng, Jie19; Kellermann, Hanna16,17; Riffeser, Arno17; Wang, Liang14,15,18; Collins, Karen A.13; Bieryla, Allyson13; Buchhave, Lars A.1; Howell, Steve B.12
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2024-03-01
卷号24期号:3页码:035012
关键词planets and satellites: fundamental parameters planets and satellites: gaseous planets stars: fundamental parameters stars: low-mass methods: data analysis techniques: photometric techniques: spectroscopic
ISSN号1674-4527
DOI10.1088/1674-4527/ad057b
产权排序17
英文摘要We report the confirmation of a sub-Saturn-size exoplanet, TOI-1194 b with a mass about 0.456(-0.051)(+0.055) MJ, and a very low mass companion star with a mass of about 96.5 +/- 1.5 M-J, TOI-1251 B. Exoplanet candidates provided by the Transiting Exoplanet Survey Satellite (TESS) are suitable for further follow-up observations by ground-based telescopes with small and medium apertures. The analysis is performed based on data from several telescopes worldwide, including telescopes in the Sino-German multiband photometric campaign, which aimed at confirming TESS Objects of Interest (TOIs) using ground-based small-aperture and medium-aperture telescopes, especially for long-period targets. TOI-1194 b is confirmed based on the consistent periodic transits depths from the multiband photometric data. We measure an orbital period of 2.310644 +/- 0.000001 d, and radius is 0.767(-0.041 )(+0.045)RJ, and amplitude of RV curve is 69.4(-7.3)(+7.9) m/s(-1). TOI-1251 B is confirmed based on the multiband photometric and high-resolution spectroscopic data, whose orbiting period is 5.963054(-0.000001)(+0.000002) d, the radius is 0.947(-0.033)(+0.035) RJ, and amplitude of RV curve is 9849(-40 )(+42)m/s(-1).
WOS关键词PHOTOMETRIC SYSTEM ; SPECKLE OBSERVATIONS ; PLANET ; KEPLER ; TELESCOPE ; ASTROPY ; PACKAGE ; PROJECT ; CAMERA ; RADII
资助项目National Natural Science Foundation of China (NSFC)[U1831209] ; National Natural Science Foundation of China (NSFC)[U2031144] ; Ankara University (BAP)[18A0759001] ; NASA's Science Mission directorate[SG2] ; TESS Science Office (TSO) ; NASA High-End Computing (HEC) Program through the NASA
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001176661500001
出版者NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
资助机构National Natural Science Foundation of China (NSFC) ; Ankara University (BAP) ; NASA's Science Mission directorate ; TESS Science Office (TSO) ; NASA High-End Computing (HEC) Program through the NASA
源URL[http://ir.xao.ac.cn/handle/45760611-7/5911]  
专题研究单元未命名
通讯作者Grupp, Frank; Wang, Hui-Juan
作者单位1.Tech Univ Denmark, Natl Space Inst, DK-2800 Lyngby, Denmark
2.Lijiang Gemini Observ, Lijiang 674199, Peoples R China
3.Urumqi 1 Sr High Sch, Urumqi 830002, Peoples R China
4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
5.Ankara Univ, Dept Astron & Space Sci, TR-06100 Ankara, Turkiye
6.Univ La Laguna, Dept Astrofis, San Cristobal la Laguna, Tenerife, Spain
7.Inst Astrofis Canarias IAC, E-38205 San Cristobal la Laguna, Tenerife, Spain
8.Swarthmore Coll, Dept Phys & Astron, Swarthmore, PA 19081 USA
9.Washington Univ, Dept Phys, St Louis, MO 63130 USA
10.Grand Pra Observ, Valais Sion, Switzerland
推荐引用方式
GB/T 7714
Wang, Jia-Qi,Jiang, Xiao-Jun,Zheng, Jie,et al. Confirmation of a Sub-Saturn-size Transiting Exoplanet Orbiting a G Dwarf: TOI-1194 b and a Very Low Mass Companion Star: TOI-1251 B from TESS[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2024,24(3):035012.
APA Wang, Jia-Qi.,Jiang, Xiao-Jun.,Zheng, Jie.,Kellermann, Hanna.,Riffeser, Arno.,...&Wang, Hui-Juan.(2024).Confirmation of a Sub-Saturn-size Transiting Exoplanet Orbiting a G Dwarf: TOI-1194 b and a Very Low Mass Companion Star: TOI-1251 B from TESS.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,24(3),035012.
MLA Wang, Jia-Qi,et al."Confirmation of a Sub-Saturn-size Transiting Exoplanet Orbiting a G Dwarf: TOI-1194 b and a Very Low Mass Companion Star: TOI-1251 B from TESS".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 24.3(2024):035012.

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