The Discovery of Five Hot Jupiters by TESS

dc.contributor.authorGuenther,Eike W.
dc.contributor.authorCochran,William D.
dc.contributor.authorMacQueen,Phillip J.
dc.contributor.authorGoffo,Elisa
dc.contributor.authorKellermann,Hanna
dc.contributor.authorNsamba,Benard
dc.contributor.authorEndl,Michael
dc.contributor.authorSebastian,Daniel
dc.contributor.authorGandolf,Davide
dc.contributor.authorAumasson,Cyrille
dc.contributor.authorBarragán,Oscar
dc.contributor.authorBednarz,Slawomir
dc.contributor.authorBernacki,Krzysztof
dc.contributor.authorBieryla,Allyson
dc.contributor.authorCiardi,David R.
dc.contributor.authorClark,Catherine A.
dc.contributor.authorsizmadia,Szilard C
dc.contributor.authorDeeg,Hans J.
dc.contributor.authorDuke,Parker
dc.contributor.authorGeorgieva,Iskra
dc.contributor.authorGrupp,Frank
dc.contributor.authorMuheki,Priscilla
dc.contributor.authorMurgas,Felipe
dc.contributor.authorNarita,Norio
dc.contributor.authorOlmschenk,Greg
dc.contributor.authorSerrano,Luisa Maria
dc.contributor.authorEylen,Vincent Van
dc.contributor.authorEyken,Julian Van
dc.contributor.authorWünsche,Anäel
dc.date.accessioned2026-09-04T10:58:25Z
dc.date.issued2026
dc.description.abstractDespite decades of research on hot Jupiters, there are still several theories for their formation. Perhaps hot Jupiters form in several ways. Atmospheric and dynamical studies have the capability to constrain the formation scenarios. However, potential targets have to be well characterized before these observations can further constrain the theories. We present the confirmation and characterization of five hot and warm Jupiters discovered by the TESS space mission. Using TESS data combined with ground-based observations, we determine the masses, radii, and other parameters of TOI-2040 b, TOI-2049 b, TOI-2578 b, TOI-4427 b, and TOI-4458 b. Three of the planets have equilibrium temperatures of about 1800 K while two have temperatures of about 1000 K. Particularly interesting for future atmospheric characterizations are TOI-2578 b and TOI-4427 b, because of their low density and large transmission spectroscopy metric. TOI-4458 b is of special interest because it is in the northern PLATO field. It appears that TOI-2040 b has a small, but measurable eccentricity
dc.identifier.citationGuenther, E. W., Cochran, W. D., MacQueen, P. J., Goffo, E., Kellermann, H., Nsamba, B., ... & Wünsche, A. (2026). The Discovery of Five Hot Jupiters by TESS. The Astronomical Journal, 172(1), 54.
dc.identifier.urihttps://ir.must.ac.ug/handle/123456789/4538
dc.language.isoen_US
dc.publisherThe Astronomical Journal
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 United Statesen
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/us/
dc.subjecthot Jupiters
dc.titleThe Discovery of Five Hot Jupiters by TESS
dc.typeArticle

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