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The ESO SupJup Survey. III. Confirmation of 13CO in YSES 1 b and Atmospheric Detection of YSES 1 c with CRIRES+

  • Authors: Yapeng Zhang, Darío González Picos, Sam de Regt, Ignas A. G. Snellen, Siddharth Gandhi, Christian Ginski, Aurora Y. Kesseli, Rico Landman, Paul Mollière, Evert Nasedkin, Alejandro Sánchez-López, Tomas Stolker, Julie Inglis, Heather A. Knutson, Dimitri Mawet, Nicole Wallack, Jerry W. Xuan

Yapeng Zhang et al 2024 The Astronomical Journal 168 .

  • Provider: AAS Journals

Caption: Figure 7.

Posterior distribution of retrieved parameters for YSES 1 c, including surface gravity, effective temperature, C/O ratio, metallicity, and quenching pressure. The vertical dashed lines denote the medium and 1σ intervals. The upper right-hand panel shows the retrieved 1σ, 2σ, and 3σ envelope of the TP profile. The dotted line is the flux-weighted emission contribution. The dashed line is the condensation curve of MgSiO3 clouds, located below the region of the main emission contribution.

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