The TESS Grand Unified Hot Jupiter Survey. III. Thirty More Giant Planets<sup>*</sup>

Yee, S.W.; Winn, J.N.; Hartman, J.D.; Rodriguez, J.E.; Zhou, G.; Latham, D.W.; Quinn, S.N.; Bieryla, A.; Collins, K.A.; Eastman, J.D.; Collins, K.I.; Conti, D.M.; Jensen Eric, L.N.; Baker, D.; Barkaoui, K.; Baştürk, Ö.; Battley, M.P.; Bayliss, D.; Beatty, T.G.; Beletsky, Y.; Belinski, A.A.; Benkhaldoun, Z.; Benni, P.; Bosch-Cabot, P.; Briceño, C.; Brudny, A.; Burleigh, M.R.; Butler, R.P.; Chairetas, S.; Chontos, A.; Christiansen, J.; Ciardi, D.R.; Clark, C.A.; Cloutier, R.; Craig, M.W.; Crane, J.D.; Dowling, N.; Dressing, C.D.; Emmanuel, J.; Evans, P.; Everett, M.E.; Fernández-Rodríguez, G.; Fernández, F.J.; Forés-Toribio, R.; Fortenbach, C.D.; Fukui, A.; Furlan, E.; Gan, T.; Ghachoui, M.; Giacalone, S.; Gill, S.; Gillon, M.; Hall, K.; Hayashi, Y.; Hedges, C.; Higuera, J.; Hintz, E.G.; Hirsch, L.; Holcomb, R.; Horne, K.; Grau, H.F.; Howard, A.W.; Howell, S.B.; Isaacson, H.; Jenkins, J.M.; Kagetani, T.; Kamler, J.; Kendall, A.; Korth, J.; Kroft, M.A.; Lacedelli, G.; Laloum, D.; Law, N.; de Leon, J.P.; Levine, A.M.; Lewin, P.; Logsdon, S.E.; Lund, M.B.; Madsen, M.M.; Mann, A.W.; Mann, C.R.; Maslennikova, N.A.; Matutano, S.; McCormack, M.; McLeod, K.K.; Michaels, E.J.; Mireles, I.; Mori, M.; Muñoz, J.A.; Murgas, F.; Narita, N.; O’Brien, S.M.; Odden, C.; Palle, E.; Patel, Y.G.; Plavchan, P.; Polanski, A.S.; Popowicz, A.; Radford, D.J.; Reed, P.A.; Relles, H.M.; Rice, M.; Ricker, G.R.; Safonov, B.S.; Savel, A.B.; Schulte, J.; Schwarz, R.P.; Schweiker, H.; Seager, S.; Sefako, R.; Shectman, S.A.; Shporer, A.; Stephens, D.C.; Stockdale, C.; Striegel, S.; Tan, T.; Teske, J.K.; Timmermans, M.; Ulmer-Moll, S.; Wang, G.; Wheatley, P.J.; Yalcinkaya, S.; Zambelli, R.; Van Zandt, J.; Ziegler, C.

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Дата последнего поиска статьи во внешних источниках: 8 октября 2025 г.

Авторы: Yee Samuel W., Winn Joshua N., Hartman Joel D., Rodriguez Joseph E., Zhou George, Latham David W., Quinn Samuel N., Bieryla Allyson, Collins Karen A., Eastman Jason D., Collins Kevin I., Conti Dennis M., Jensen Eric L.N., Baker David, Barkaoui Khalid, Baştürk Özgür, Battley Matthew P., Bayliss Daniel, Beatty Thomas G., Beletsky Yuri, Belinski Alexander A., Benkhaldoun Zouhair, Benni Paul, Bosch-Cabot Pau, Briceño César, Brudny Andrzej, Burleigh Matthew R., Butler R.Paul, Chairetas Stavros, Chontos Ashley, Christiansen Jessie, Ciardi David R., Clark Catherine A., Cloutier Ryan, Craig Matthew W., Crane Jeffrey D., Dowling Nicholas, Dressing Courtney D., Emmanuel Jehin, Evans Phil, Everett Mark E., Fernández-Rodríguez Gareb, Fernández Fernández Jorge, Forés-Toribio Raquel, Fortenbach Charles D., Fukui Akihiko, Furlan Elise, Gan Tianjun, Ghachoui Mourad, Giacalone Steven, Gill Samuel, Gillon Michaël, Hall Kylie, Hayashi Yuya, Hedges Christina, Higuera Jesus, Hintz Eric G., Hirsch Lea, Holcomb Rae, Horne Keith, Grau Horta Ferran, Howard Andrew W., Howell Steve B., Isaacson Howard, Jenkins Jon M., Kagetani Taiki, Kamler Jacob, Kendall Alicia, Korth Judith, Kroft Maxwell A., Lacedelli Gaia, Laloum Didier, Law Nicholas, de Leon Jerome Pitogo, Levine Alan M., Lewin Pablo, Logsdon Sarah E., Lund Michael B., Madsen Madelyn M., Mann Andrew W., Mann Christopher R., Maslennikova Nataliia A., Matutano Sandra, McCormack Mason, McLeod Kim K., Michaels Edward J., Mireles Ismael, Mori Mayuko, Muñoz Jose A., Murgas Felipe, Narita Norio, O’Brien Sean M., Odden Caroline, Palle Enric, Patel Yatrik G., Plavchan Peter, Polanski Alex S., Popowicz Adam, Radford Don J., Reed Phillip A., Relles Howard M., Rice Malena, Ricker George R., Safonov Boris S., Savel Arjun B., Schulte Jack, Schwarz Richard P., Schweiker Heidi, Seager Sara, Sefako Ramotholo, Shectman Stephen A., Shporer Avi, Stephens Denise C., Stockdale Chris, Striegel Stephanie, Tan Thiam-Guan, Teske Johanna K., Timmermans Mathilde, Ulmer-Moll Solène, Wang Gavin, Wheatley Peter J., Yalcinkaya Selçuk, Zambelli Roberto, Van Zandt Judah, Ziegler Carl
Журнал: Astrophysical Journal, Supplement Series
Том: 280
Номер: 1
Год издания: 2025
Издательство: University of Chicago Press
Местоположение издательства: United States
Первая страница: 1
Последняя страница: 41
Номер статьи: 30
DOI: 10.3847/1538-4365/aded0d
Аннотация: We present the discovery of 30 transiting giant planets that were initially detected using data from NASA's Transiting Exoplanet Survey Satellite mission. These new planets orbit relatively bright (G ≤ 12.5) FGK host stars with orbital periods between 1.6 and 8.2 days, and have radii between 0.9 and 1.7 Jupiter radii. We performed follow-up ground-based photometry, high angular resolution imaging, high-resolution spectroscopy, and radial velocity monitoring for each of these objects to confirm that they are planets and determine their masses and other system parameters. The planets' masses span more than an order of magnitude (0.17 MJ < Mp < 3.3 MJ). For two planets, TOI-3593 b and TOI-4961 b, we measured significant nonzero eccentricities of 0.11‑0.03+0.05 and 0.18‑0.05+0.04 , respectively, while for the other planets, the data typically provide a 1σ upper bound of 0.15 on the eccentricity. These discoveries represent a major step toward assembling a complete, magnitude-limited sample of transiting hot Jupiters around FGK stars. *This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile.
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The TESS Grand Unified Hot Jupiter Survey. III. Thirty More Giant Planets<sup>*</sup>статья

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