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Unraveling the Mystery of the Peculiar and Young Hot Jupiter CoRoT-2 b. II. Phase-resolved Emission Spectroscopy with Very Large Telescope/CRIRES+ and Gemini South/IGRINS

  • Authors: Aurora Y. Kesseli, Siddharth Gandhi, Lisa Dang, Alexis Lavail, Alejandro Sánchez-López, Ying Shu, Emily Rauscher, Hayley Beltz, Romain Allart, Stefan Pelletier, Vatsal Panwar

Aurora Y. Kesseli et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 11.

Corner plot showing the posterior distribution of all inferred parameters from the nominal atmospheric retrieval, which included major C- and O-bearing species expected to exist in a CoRoT-2 b-like planet. The model also includes a uniform gray cloud deck and the PT profile is parameterized by a modified T. Guillot (2010) PT profile (T. Guillot & M. Havel 2011; P. Mollière et al. 2019).

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