TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full-frame Images

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dc.contributor.authorRodriguez, Joseph E.
dc.contributor.authorQuinn, Samuel N.
dc.contributor.authorZhou, George
dc.contributor.authorVanderburg, Andrew
dc.contributor.authorNielsen, Louise D.
dc.contributor.authorWittenmyer, Robert A.
dc.contributor.authorBrahm, Rafael
dc.contributor.authorReed, Phillip A.
dc.contributor.authorHuang, Chelsea X.
dc.contributor.authorVach, Sydney
dc.contributor.authorCiardi, David R.
dc.contributor.authorOelkers, Ryan J.
dc.contributor.authorStassun, Keivan G.
dc.contributor.authorHellier, Coel
dc.contributor.authorGaudi, B. Scott
dc.contributor.authorEastman, Jason D.
dc.contributor.authorCollins, Karen A.
dc.contributor.authorBieryla, Allyson
dc.contributor.authorChristian, Sam
dc.contributor.authorLatham, David W.
dc.contributor.authorCarleo, Ilaria
dc.contributor.authorWright, Duncan J.
dc.contributor.authorMatthews, Elisabeth
dc.contributor.authorGonzales, Erica J.
dc.contributor.authorZiegler, Carl
dc.contributor.authorDressing, Courtney D.
dc.contributor.authorHowell, Steve B.
dc.contributor.authorTan, Thiam-Guan
dc.contributor.authorWittrock, Justin
dc.contributor.authorPlavchan, Peter
dc.contributor.authorMcLeod, Kim K.
dc.contributor.authorBaker, David
dc.contributor.authorWang, Gavin
dc.contributor.authorRadford, Don J.
dc.contributor.authorSchwarz, Richard P.
dc.contributor.authorEsposito, Massimiliano
dc.contributor.authorRicker, George R.
dc.contributor.authorVanderspek, Roland K.
dc.contributor.authorSeager, Sara
dc.contributor.authorWinn, Joshua N.
dc.contributor.authorJenkins, Jon M.
dc.contributor.authorAddison, Brett
dc.contributor.authorAnderson, D. R.
dc.contributor.authorBarclay, Thomas
dc.contributor.authorBeatty, Thomas G.
dc.contributor.authorBerlind, Perry
dc.contributor.authorBouchy, Francois
dc.contributor.authorBowen, Michael
dc.contributor.authorBowler, Brendan P.
dc.contributor.authorBrasseur, C. E.
dc.contributor.authorBriceno, Cesar
dc.contributor.authorCaldwell, Douglas A.
dc.contributor.authorCalkins, Michael L.
dc.contributor.authorCartwright, Scott
dc.contributor.authorChaturvedi, Priyanka
dc.contributor.authorChaverot, Guillaume
dc.contributor.authorChimaladinne, Sudhish
dc.contributor.authorChristiansen, Jessie L.
dc.contributor.authorCollins, Kevin I.
dc.contributor.authorCrossfield, Ian J. M.
dc.contributor.authorEastridge, Kevin
dc.contributor.authorEspinoza, Nestor
dc.contributor.authorEsquerdo, Gilbert A.
dc.contributor.authorFeliz, Dax L.
dc.contributor.authorFenske, Tyler
dc.contributor.authorFong, William
dc.contributor.authorGan, Tianjun
dc.contributor.authorGiacalone, Steven
dc.contributor.authorGill, Holden
dc.contributor.authorGordon, Lindsey
dc.contributor.authorGranados, A.
dc.contributor.authorGrieves, Nolan
dc.contributor.authorGuenther, Eike W.
dc.contributor.authorGuerrero, Natalia
dc.contributor.authorHenning, Thomas
dc.contributor.authorHenze, Christopher E.
dc.contributor.authorHesse, Katharine
dc.contributor.authorHobson, Melissa J.
dc.contributor.authorHorner, Jonathan
dc.contributor.authorJames, David J.
dc.contributor.authorJensen, Eric L. N.
dc.contributor.authorJimenez, Mary
dc.contributor.authorJordan, Andres
dc.contributor.authorKane, Stephen R.
dc.contributor.authorKielkopf, John
dc.contributor.authorKim, Kingsley
dc.contributor.authorKuhn, Rudolf B.
dc.contributor.authorLatouf, Natasha
dc.contributor.authorLaw, Nicholas M.
dc.contributor.authorLevine, Alan M.
dc.contributor.authorLund, Michael B.
dc.contributor.authorMann, Andrew W.
dc.contributor.authorMao, Shude
dc.contributor.authorMatson, Rachel A.
dc.contributor.authorMengel, Matthew W.
dc.contributor.authorMink, Jessica
dc.contributor.authorNewman, Patrick
dc.contributor.authorO'Dwyer, Tanner
dc.contributor.authorOkumura, Jack
dc.contributor.authorPalle, Enric
dc.contributor.authorPepper, Joshua
dc.contributor.authorQuintana, Elisa V.
dc.contributor.authorSarkis, Paula
dc.contributor.authorSavel, Arjun B.
dc.contributor.authorSchlieder, Joshua E.
dc.contributor.authorSchnaible, Chloe
dc.contributor.authorShporer, Avi
dc.contributor.authorSefako, Ramotholo
dc.contributor.authorSeidel, Julia V.
dc.contributor.authorSiverd, Robert J.
dc.contributor.authorSkinner, Brett
dc.contributor.authorStalport, Manu
dc.contributor.authorStevens, Daniel J.
dc.contributor.authorStibbards, Caitlin
dc.contributor.authorTinney, C. G.
dc.contributor.authorWest, R. G.
dc.contributor.authorYahalomi, Daniel A.
dc.contributor.authorZhang, Hui
dc.date.accessioned2025-01-20T23:52:03Z
dc.date.available2025-01-20T23:52:03Z
dc.date.issued2021
dc.description.abstractWe 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 (R-P = 1.01-1.77 R-J) and have masses that range from 0.85 to 6.33 M-J. The host stars of these systems have F and G spectral types (5595 <= T-eff <= 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 (log g < 4.1). TOI-640 b is one of only three known hot Jupiters to have a highly inflated radius (R-P > 1.7 R-J, 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) M-J 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.
dc.fuente.origenWOS
dc.identifier.doi10.3847/1538-3881/abe38a
dc.identifier.eissn1538-3881
dc.identifier.issn0004-6256
dc.identifier.urihttps://doi.org/10.3847/1538-3881/abe38a
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/94878
dc.identifier.wosidWOS:000632893600001
dc.issue.numero4
dc.language.isoen
dc.revistaAstronomical journal
dc.rightsacceso restringido
dc.subjectExoplanet astronomy
dc.subjectExoplanet migration
dc.subjectExoplanet detection methods
dc.subjectExoplanets
dc.subjectTransits
dc.subjectRadial velocity
dc.subjectDirect imaging
dc.subject.ods13 Climate Action
dc.subject.odspa13 Acción por el clima
dc.titleTESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full-frame Images
dc.typeartículo
dc.volumen161
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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