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Photochemical Production of CS2 in Temperate-to-warm Gas Giant Exoplanet Atmospheres

  • Authors: Jeehyun Yang, Vighnesh Nagpal, Michael Zhang, Qiao Xue, Eliza M.-R. Kempton, Jacob L. Bean, Michael R. Line, Jonathan J. Fortney, Peter Gao, Matthew C. Nixon, Caroline Piaulet-Ghorayeb, Kevin B. Stevenson, Madison Brady, Joost P. Wardenier, Luis Welbanks, Jean-Michel Désert, Guangwei Fu, Vivien Parmentier, Diana Powell

Jeehyun Yang et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 3.

Sensitivity analysis of the atmosphere of TOI-6894 b for various model input parameters. The reference model assumes Kzz = 108 cm2 s−1, 1× Z⊙ metallicity, and Tint = 100 K. The model parameters were varied for (a) Kzz, (b) metallicity, and (c) Tint. Colors denote different chemical species, while line styles indicate the values adopted for the varied parameter in each panel. Solid lines correspond to the reference model. Tint has the smallest effect on CS2 formation among the parameters considered.

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