April
2021
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2021AJ....161..194R
Authors
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Rodriguez, Joseph E.
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Quinn, Samuel N.
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Zhou, George
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Vanderburg, Andrew
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Nielsen, Louise D.
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Wittenmyer, Robert A.
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Brahm, Rafael
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Reed, Phillip A.
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Huang, Chelsea X.
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Vach, Sydney
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Ciardi, David R.
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Oelkers, Ryan J.
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Stassun, Keivan G.
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Hellier, Coel
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Gaudi, B. Scott
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Eastman, Jason D.
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Collins, Karen A.
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Bieryla, Allyson
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Christian, Sam
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Latham, David W.
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Carleo, Ilaria
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Wright, Duncan J.
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Matthews, Elisabeth
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Gonzales, Erica J.
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Ziegler, Carl
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Dressing, Courtney D.
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Howell, Steve B.
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Tan, Thiam-Guan
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Wittrock, Justin
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Plavchan, Peter
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McLeod, Kim K.
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Baker, David
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Wang, Gavin
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Radford, Don J.
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Schwarz, Richard P.
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Esposito, Massimiliano
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Ricker, George R.
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Vanderspek, Roland K.
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Seager, Sara
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Winn, Joshua N.
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Jenkins, Jon M.
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Addison, Brett
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Anderson, D. R.
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Barclay, Thomas
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Beatty, Thomas G.
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Berlind, Perry
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Bouchy, Francois
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Bowen, Michael
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Bowler, Brendan P.
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Brasseur, C. E.
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Briceño, César
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Caldwell, Douglas A.
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Calkins, Michael L.
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Cartwright, Scott
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Chaturvedi, Priyanka
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Chaverot, Guillaume
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Chimaladinne, Sudhish
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Christiansen, Jessie L.
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Collins, Kevin I.
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Crossfield, Ian J. M.
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Eastridge, Kevin
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Espinoza, Néstor
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Esquerdo, Gilbert A.
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Feliz, Dax L.
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Fenske, Tyler
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Fong, William
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Gan, Tianjun
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Giacalone, Steven
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Gill, Holden
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Gordon, Lindsey
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Granados, A.
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Grieves, Nolan
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Guenther, Eike W.
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Guerrero, Natalia
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Henning, Thomas
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Henze, Christopher E.
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Hesse, Katharine
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Hobson, Melissa J.
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Horner, Jonathan
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James, David J.
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Jensen, Eric L. N.
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Jimenez, Mary
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Jordán, Andrés
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Kane, Stephen R.
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Kielkopf, John
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Kim, Kingsley
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Kuhn, Rudolf B.
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Latouf, Natasha
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Law, Nicholas M.
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Levine, Alan M.
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Lund, Michael B.
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Mann, Andrew W.
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Mao, Shude
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Matson, Rachel A.
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Mengel, Matthew W.
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Mink, Jessica
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Newman, Patrick
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O'Dwyer, Tanner
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Okumura, Jack
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Palle, Enric
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Pepper, Joshua
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Quintana, Elisa V.
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Sarkis, Paula
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Savel, Arjun B.
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Schlieder, Joshua E.
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Schnaible, Chloe
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Shporer, Avi
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Sefako, Ramotholo
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Seidel, Julia V.
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Siverd, Robert J.
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Skinner, Brett
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Stalport, Manu
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Stevens, Daniel J.
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Stibbards, Caitlin
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Tinney, C. G.
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West, R. G.
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Yahalomi, Daniel A.
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Zhang, Hui
Abstract
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We present the discovery and characterization of five hot and warm Jupiters—TOI-628 b (TIC 281408474; HD 288842), TOI-640 b (TIC 147977348), TOI-1333 b (TIC 395171208, BD+47 3521A), TOI-1478 b (TIC 409794137), and TOI-1601 b (TIC 139375960)—based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The five planets were identified from the full-frame images and were confirmed through a series of photometric and spectroscopic follow-up observations by the TESS Follow-up Observing Program Working Group. The planets are all Jovian size (RP = 1.01-1.77 RJ) and have masses that range from 0.85 to 6.33 MJ. The host stars of these systems have F and G spectral types (5595 ≤ Teff ≤ 6460 K) and are all relatively bright (9.5 < V < 10.8, 8.2 < K < 9.3), making them well suited for future detailed characterization efforts. Three of the systems in our sample (TOI-640 b, TOI-1333 b, and TOI-1601 b) orbit subgiant host stars ( $\mathrm{log}$ g < 4.1). TOI-640 b is one of only three known hot Jupiters to have a highly inflated radius (RP > 1.7 RJ, possibly a result of its host star's evolution) and resides on an orbit with a period longer than 5 days. TOI-628 b is the most massive, hot Jupiter discovered to date by TESS with a measured mass of ${6.31}_{-0.30}^{+0.28}$ MJ and a statistically significant, nonzero orbital eccentricity of e = ${0.074}_{-0.022}^{+0.021}$ . This planet would not have had enough time to circularize through tidal forces from our analysis, suggesting that it might be remnant eccentricity from its migration. The longest-period planet in this sample, TOI-1478 b (P = 10.18 days), is a warm Jupiter in a circular orbit around a near-solar analog. NASA's TESS mission is continuing to increase the sample of well-characterized hot and warm Jupiters, complementing its primary mission goals.
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