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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 8.

Comparison between the 1D CCFs resulting from the cross correlation between the artificially broadened models and the unbroadened model (dashed lines) vs. the data with the same unbroadened model (black solid line). The models were broadened with a ﹩v\sin (i)﹩ kernel and correspond to ﹩v\sin (i)﹩ values from 0 to 12 km s−1. The models and the data have all been normalized so that their peak values are at one so that the widths of the lines can be compared more easily. The width of the CCF made using the CRIRES+ data falls between the profiles of the 0 and 3 km s–1 ﹩v\sin (i)﹩ models, and we determine a ﹩v\sin (i)﹩ of 2.1 km s−1 using this method.

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