论文标题

TOI-2046b,TOI-1181B和TOI-1516B,来自\ textit {tess}的三个新的热木星:行星绕着年轻恒星,一个子巨星和一个普通星星

TOI-2046b, TOI-1181b and TOI-1516b, three new hot Jupiters from \textit{TESS}: planets orbiting a young star, a subgiant and a normal star

论文作者

Kabáth, Petr, Chaturvedi, Priyanka, MacQueen, Phillip J., Skarka, Marek, Šubjak, Ján, Esposito, Massimilliano, Cochran, William D., Bellomo, Salvatore E., Karjalainen, Raine, Guenther, Eike W., Endl, Michael, Csizmadia, Szilárd, Karjalainen, Marie, Hatzes, Artie, Žák, Jiří, Gandolfi, Davide, Boffin, Henri M. J., Vines, Jose I., Livingston, John H., García, Rafael A., Mathur, Savita, González-Cuesta, Lucía, Blažek, Martin, Caldwell, Douglas A., Colón, Knicole D., Deeg, Hans, Erikson, Anders, Van Eylen, Vincent, Fong, William, Fridlund, Malcolm, Fukui, Akihiko, Fűrész, Gábor, Goeke, Robert F., Goffo, Elisa, Howell, Steve, Jenkins, Jon M., Klagyivik, Peter, Korth, Judith, Latham, David W., Luque, Rafael, Moldovan, Dan, Murgas, Felipe, Narita, Norio, Orell-Miquel, Jaume, Palle, Enric, Parviainen, Hannu, Persson, Carina M., Reed, Phillip A., Redfield, Seth, Ricker, George R., Seager, Sara, Serrano, Luisa Maria, Shporer, Avi, Smith, Alexis M. S., Watanabe, Noriharu, Winn, Joshua N., team, the KESPRINT

论文摘要

我们介绍了由苔丝太空任务发现的三个热木星,TOI-1181b,TOI-1516B和TOI-2046b的确认和表征。据报道的热木星的轨道周期在1.4至2.05天之间。这三个行星的质量为$ 1.18 \ pm0.14 $ m $ _ {\ mathrm {j}} $,$ 3.16 \ pm0.12 $ \,m $ _ {\ mathrm {j}} $ TOI-1516B和TOI-2046b。 TOI-1181b的恒星宿主是F9IV恒星,而TOI-1516b和TOI-2046b轨道F主序列宿主星。前两个系统的年龄在2-5个回旋范围内。但是,TOI-2046是拥有热木星的少数最年轻的行星系统之一,年龄估计为100-400 MYR。这三个行星的径向速度随访所使用的主要仪器位于Ondčjov,Tautenburg和McDonald天文台,所有三个行星都安装在2-3米的孔径望远镜上,表明中端望远镜网络可以在巨大的巨大望远镜中发挥重要作用。 \ textit {plato}。

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. 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 meter aperture telescopes, demonstrating that mid-aperture telescope networks can play a substantial role in the follow-up of gas giants discovered by \textit{TESS} and in the future by \textit{PLATO}.

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