NGTS-30 B/toi-4862 B: an 1 Gyr Old 98-Day Transiting Warm Jupiter

M. P. Battley,K. A. Collins,S. Ulmer-Moll,S. N. Quinn,M. Lendl,S. Gill,R. Brahm,M. J. Hobson,H. P. Osborn,A. Deline,J. P. Faria, A. B. Claringbold,H. Chakraborty,K. G. Stassun,C. Hellier, D. R. Alves,C. Ziegler,D. R. Anderson, I. Apergis, D. J. Armstrong,D. Bayliss,Y. Beletsky,A. Bieryla,F. Bouchy,M. R. Burleigh,R. P. Butler,S. L. Casewell,J. L. Christiansen,J. D. Crane,P. A. Dalba,T. Daylan,P. Figueira,E. Gillen,M. R. Goad,M. N. Guenther,B. A. Henderson,T. Henning,J. S. Jenkins,A. Jordan,S. Kanodia,A. Kendall,M. Kunimoto,D. W. Latham,A. M. Levine,J. Mccormac,M. Moyano,A. Osborn,D. Osip, T. A. Pritchard,A. Psaridi, M. Rice,J. E. Rodriguez, S. Saha,S. Seager,S. A. Shectman,A. M. S. Smith,J. K. Teske,E. B. Ting,S. Udry,J. I. Vines,C. A. Watson,R. G. West,P. J. Wheatley,J. N. Winn, S. W. Yee, Y. Zhao

Astronomy and Astrophysics（2024）

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关键词

methods: data analysis,planets and satellites: detection,planets and satellites: gaseous planets,planets and satellites: general,planets and satellites: individual: NGTS-30 b,planets and satellites: individual: TOI-4862 b

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