TOI-2046b, TOI-1181b, and TOI-1516b, three new hot Jupiters from TESS: planets orbiting a young star, a subgiant, and a normal star
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KABÁTH, Petr; Priyanka CHATURVEDI; Phillip J. MACQUEEN; Marek SKARKA; Ján ŠUBJAK; Massimilliano ESPOSITO; William D. COCHRAN; Salvatore E. BELLOMO; Raine KARJALAINEN; Eike W. GUENTHER; Michael ENDL; Szilárd CSIZMADIA; Marie KARJALAINEN; Artie HATZES; Jiří ŽÁK; Davide GANDOLFI; Henri M. J. BOFFIN; Jose I. VINES; John H. LIVINGSTON; Rafael A. GARCÍA; Savita MATHUR; Lucía GONZÁLEZ-CUESTA; Martin BLAŽEK; Douglas A. CALDWELL; Knicole D. COLÓN; Hans DEEG; Anders ERIKSON; Vincent VAN EYLEN; William FONG; Malcolm FRIDLUND; Akihiko FUKUI; Gábor FŰRÉSZ; Robert F. GOEKE; Elisa GOFFO; Steve HOWELL; Jon M. JENKINS; Peter KLAGYIVIK; Judith KORTH; David W. LATHAM; Rafael LUQUE; Dan MOLDOVAN; Felipe MURGAS; Norio NARITA; Jaume ORELL-MIQUEL; Enric PALLE; Hannu PARVIAINEN; Carina M. PERSSON; Phillip A. REED; Seth REDFIELD; George R. RICKER; Sara SEAGER; Luisa Maria SERRANO; Avi SHPORER; Alexis M. S. SMITH; Noriharu WATANABE a Joshua N. WINN
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Monthly Notices of the Royal Astronomical Society, Oxford University Press, 2022, 0035-8711
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.
KABÁTH, Petr; Priyanka CHATURVEDI; Phillip J. MACQUEEN; Marek SKARKA; Ján ŠUBJAK; Massimilliano ESPOSITO; William D. COCHRAN; Salvatore E. BELLOMO; Raine KARJALAINEN; Eike W. GUENTHER; Michael ENDL; Szilárd CSIZMADIA; Marie KARJALAINEN; Artie HATZES; Jiří ŽÁK; Davide GANDOLFI; Henri M. J. BOFFIN; Jose I. VINES; John H. LIVINGSTON; Rafael A. GARCÍA; Savita MATHUR; Lucía GONZÁLEZ-CUESTA; Martin BLAŽEK; Douglas A. CALDWELL; Knicole D. COLÓN; Hans DEEG; Anders ERIKSON; Vincent VAN EYLEN; William FONG; Malcolm FRIDLUND; Akihiko FUKUI; Gábor FŰRÉSZ; Robert F. GOEKE; Elisa GOFFO; Steve HOWELL; Jon M. JENKINS; Peter KLAGYIVIK; Judith KORTH; David W. LATHAM; Rafael LUQUE; Dan MOLDOVAN; Felipe MURGAS; Norio NARITA; Jaume ORELL-MIQUEL; Enric PALLE; Hannu PARVIAINEN; Carina M. PERSSON; Phillip A. REED; Seth REDFIELD; George R. RICKER; Sara SEAGER; Luisa Maria SERRANO; Avi SHPORER; Alexis M. S. SMITH; Noriharu WATANABE a Joshua N. WINN. TOI-2046b, TOI-1181b, and TOI-1516b, three new hot Jupiters from TESS: planets orbiting a young star, a subgiant, and a normal star. Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2022, roč. 513, č. 4, s. 5955-5972. ISSN 0035-8711. Dostupné z: https://doi.org/10.1093/mnras/stac1254.
@article{1862970, author = {Kabáth, Petr and Chaturvedi, Priyanka and MacQueen, Phillip J. and Skarka, Marek and Šubjak, Ján and Esposito, Massimilliano and Cochran, William D. and Bellomo, Salvatore E. and Karjalainen, Raine and Guenther, Eike W. and Endl, Michael and Csizmadia, Szilárd and Karjalainen, Marie and Hatzes, Artie and Žák, Jiří and Gandolfi, Davide and Boffin, Henri M. J. and Vines, Jose I. and Livingston, John H. and García, Rafael A. and Mathur, Savita and GonzálezandCuesta, Lucía and Blažek, Martin and Caldwell, Douglas A. and Colón, Knicole D. and Deeg, Hans and Erikson, Anders and Van Eylen, Vincent and Fong, William and Fridlund, Malcolm and Fukui, Akihiko and Fűrész, Gábor and Goeke, Robert F. and Goffo, Elisa and Howell, Steve and Jenkins, Jon M. and Klagyivik, Peter and Korth, Judith and Latham, David W. and Luque, Rafael and Moldovan, Dan and Murgas, Felipe and Narita, Norio and OrellandMiquel, Jaume and Palle, Enric and Parviainen, Hannu and Persson, Carina M. and Reed, Phillip A. and Redfield, Seth and Ricker, George R. and Seager, Sara and Serrano, Luisa Maria and Shporer, Avi and Smith, Alexis M. S. and Watanabe, Noriharu and Winn, Joshua N.}, article_number = {4}, doi = {https://doi.org/10.1093/mnras/stac1254}, keywords = {techniques: radial velocities; techniques: spectroscopic; planets and satellites: detection; stars: individual: TOI-1181; TOI-1516; TOI-2046}, language = {eng}, issn = {0035-8711}, journal = {Monthly Notices of the Royal Astronomical Society}, title = {TOI-2046b, TOI-1181b, and TOI-1516b, three new hot Jupiters from TESS: planets orbiting a young star, a subgiant, and a normal star}, url = {https://arxiv.org/pdf/2205.01860.pdf}, volume = {513}, year = {2022} }
TY - JOUR ID - 1862970 AU - 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. PY - 2022 TI - TOI-2046b, TOI-1181b, and TOI-1516b, three new hot Jupiters from TESS: planets orbiting a young star, a subgiant, and a normal star JF - Monthly Notices of the Royal Astronomical Society VL - 513 IS - 4 SP - 5955-5972 EP - 5955-5972 PB - Oxford University Press SN - 00358711 KW - techniques: radial velocities KW - techniques: spectroscopic KW - planets and satellites: detection KW - stars: individual: TOI-1181 KW - TOI-1516 KW - TOI-2046 UR - https://arxiv.org/pdf/2205.01860.pdf N2 - 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. ER -
KABÁTH, Petr; Priyanka CHATURVEDI; Phillip J. MACQUEEN; Marek SKARKA; Ján ŠUBJAK; Massimilliano ESPOSITO; William D. COCHRAN; Salvatore E. BELLOMO; Raine KARJALAINEN; Eike W. GUENTHER; Michael ENDL; Szilárd CSIZMADIA; Marie KARJALAINEN; Artie HATZES; Jiří ŽÁK; Davide GANDOLFI; Henri M. J. BOFFIN; Jose I. VINES; John H. LIVINGSTON; Rafael A. GARCÍA; Savita MATHUR; Lucía GONZÁLEZ-CUESTA; Martin BLAŽEK; Douglas A. CALDWELL; Knicole D. COLÓN; Hans DEEG; Anders ERIKSON; Vincent VAN EYLEN; William FONG; Malcolm FRIDLUND; Akihiko FUKUI; Gábor F$\backslash$H URÉSZ; Robert F. GOEKE; Elisa GOFFO; Steve HOWELL; Jon M. JENKINS; Peter KLAGYIVIK; Judith KORTH; David W. LATHAM; Rafael LUQUE; Dan MOLDOVAN; Felipe MURGAS; Norio NARITA; Jaume ORELL-MIQUEL; Enric PALLE; Hannu PARVIAINEN; Carina M. PERSSON; Phillip A. REED; Seth REDFIELD; George R. RICKER; Sara SEAGER; Luisa Maria SERRANO; Avi SHPORER; Alexis M. S. SMITH; Noriharu WATANABE a Joshua N. WINN. TOI-2046b, TOI-1181b, and TOI-1516b, three new hot Jupiters from TESS: planets orbiting a young star, a subgiant, and a normal star. \textit{Monthly Notices of the Royal Astronomical Society}. Oxford University Press, 2022, roč.~513, č.~4, s.~5955-5972. ISSN~0035-8711. Dostupné z: https://doi.org/10.1093/mnras/stac1254.