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 d. The masses of the three planets are 1.18 ± 0.14 MJ, 3.16 ± 0.12 MJ, and 2.30 ± 0.28 MJ, 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. However, TOI-2046 is among the few youngest known planetary systems hosting a hot Jupiter, with an age estimate of 100–400 Myrs. The main instruments used for the radial velocity follow-up of these three planets are located at Ondřejov, Tautenburg, and McDonald Observatory, and all three are mounted on 2–3 m aperture telescopes, demonstrating that mid-aperture telescope networks can play a substantial role in the follow-up of gas giants discovered by TESS and in the future by PLATO.
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Šubjak, Ján ; Sharma, Rishikesh ; Carmichael, Theron W. ; Johnson, Marshall C. ; Gonzales, Erica J. ; Matthews, Elisabeth ; Boffin, Henri M. ; Brahm, Rafael ; Chaturvedi, Priyanka ; Chakraborty, Abhijit ; et al ( , The Astronomical Journal)null (Ed.)
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Rodriguez, Joseph E. ; Quinn, Samuel N. ; Zhou, George ; Vanderburg, Andrew ; Nielsen, Louise D. ; Wittenmyer, Robert A. ; Brahm, Rafael ; Reed, Phillip A. ; Huang, Chelsea X. ; Vach, Sydney ; et al ( , The Astronomical Journal)null (Ed.)