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Ricker, Hannu Parviainen, Hans Deeg, Henri M.J. Boffin, J\\'an \\v{S}ubjak, Jaume Orell-Miquel, Ji\\v{r}\\'i \\v{Z}\\'ak, John H. Livingston, Jon M. Jenkins, Jose I. Vines, Joshua N. Winn, Judith Korth, Knicole D. Col\\'on, Luc\\'ia Gonz\\'alez-Cuesta, Luisa Maria Serrano, Malcolm Fridlund, Marek Skarka, Marie Karjalainen, Martin Bla\\v{z}ek, Massimilliano Esposito, Michael Endl, Noriharu Watanabe, Norio Narita, Peter Klagyivik, Petr Kab\\'ath, Phillip A. Reed, Phillip J. MacQueen, Priyanka Chaturvedi, Rafael A. Garc\\'ia, Rafael Luque, Raine Karjalainen, Robert F. Goeke, Salvatore E. Bellomo, Sara Seager, Savita Mathur, Seth Redfield, Steve Howell, Szil\\'ard Csizmadia, the KESPRINT team, Vincent Van Eylen, William D. Cochran, William Fong","submitted_at":"2022-05-04T02:30:04Z","abstract_excerpt":"We present the confirmation and characterization of three hot Jupiters, TOI-1181b, TOI-1516b, and TOI-2046b, discovered by the TESS space mission. The reported hot Jupiters have orbital periods between 1.4 and 2.05 days. The masses of the three planets are $1.18\\pm0.14$ M$_{\\mathrm{J}}$, $3.16\\pm0.12$\\, M$_{\\mathrm{J}}$, and 2.30 $\\pm 0.28$ M$_{\\mathrm{J}}$, for TOI-1181b, TOI-1516b, and TOI-2046b, respectively. The stellar host of TOI-1181b is a F9IV star, whereas TOI-1516b and TOI-2046b orbit F main sequence host stars. The ages of the first two systems are in the range of 2-5 Gyrs. 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