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Supersolar Metallicity and Tentative Evidence for Photochemistry on WASP-96 b from JWST and Ground-based VLT Transmission Spectroscopy

  • Authors: Michael Radica, Jake Taylor, Yoav Rotman, Jasmina Blecic, Luis Welbanks, Eva-Maria Ahrer, Duncan Christie, Louis-Philippe Coulombe, Gillis Lowry, Matthew M. Murphy, Adina D. Feinstein, David Lafrenière, Ryan J. MacDonald, Nathan J. Mayne, Shang-Min Tsai, Maria Zamyatina

Michael Radica et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 6.

Elemental abundances and ratios in the atmosphere of WASP-96 b. Top row: derived elemental abundances for WASP-96 b’s atmosphere from each retrieval code (colored points) normalized to stellar values (N. K. Nikolov et al. 2022). For bounded constraints, the posterior median and 1σ confidence interval are shown. Otherwise, 3σ upper limits are plotted. The approximate locations of Jupiter and Saturn (sourced from S. K. Atreya et al. 2022) are marked with bold letters. Bottom row: abundance ratios derived from the above elemental constraints.

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