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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 5.

2D cross-correlation grid for the CRIRES+ Visit 2 dataset in Earth’s rest frame. Each row is a resulting CCF between the model spectra of CoRoT-2 b that contained CO and H2O and a cleaned time-series spectrum. Larger residual amplitudes indicate positive correlation between the model and the data. The horizontal violet dashed line indicates the end of secondary eclipse, while the yellow dashed lines show the planet’s expected velocity. A faint region of increased residual amplitudes between the gold dashed lines shows that the planet is detected.

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