Retrieving day- and nightside atmospheric properties of the ultra-hot Jupiter TOI-2109b: Detection of Fe and CO emission lines and evidence for inefficient heat transport.

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Bibliographic Details
Title: Retrieving day- and nightside atmospheric properties of the ultra-hot Jupiter TOI-2109b: Detection of Fe and CO emission lines and evidence for inefficient heat transport.
Authors: Cont, D.1,2 (AUTHOR) david.cont@lmu.de, Nortmann, L.3 (AUTHOR), Lesjak, F.3 (AUTHOR), Yan, F.4 (AUTHOR), Shulyak, D.5 (AUTHOR), Lavail, A.6 (AUTHOR), Stangret, M.7 (AUTHOR), Pallé, E.8,9 (AUTHOR), Amado, P. J.5 (AUTHOR), Caballero, J. A.10 (AUTHOR), Hatzes, A.11 (AUTHOR), Henning, Th.12 (AUTHOR), Piskunov, N.13 (AUTHOR), Quirrenbach, A.14 (AUTHOR), Reiners, A.3 (AUTHOR), Ribas, I.15,16 (AUTHOR), Agüí Fernández, J. F.17 (AUTHOR), Akın, C.1,18 (AUTHOR), Boldt-Christmas, L.13 (AUTHOR), Chaturvedi, P.11,19 (AUTHOR)
Source: Astronomy & Astrophysics / Astronomie et Astrophysique. 2025, Vol. 698, p1-16. 16p.
Database: Academic Search Ultimate
Description
ISSN:00046361
DOI:10.1051/0004-6361/202554572