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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 3.

Time-series spectra for a single CRIRES+ order, showing an example of the cleaning steps that were undertaken and the final spectrum. The top panel shows the pipeline-reduced spectrum after a normalization, sigma clipping, and application of a high-pass filter. The spectrum in the middle panel show the spectrum after the deepest tellurics were masked and the average spectrum in time was removed. The main features that can be seen at this point are residuals from the shallower tellurics. The bottom panel shows our final cleaned spectrum, after applying the SYSREM algorithm and masking out any columns that had large standard deviations.

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