Image Details

Choose export citation format:

GEMS JWST: Transmission Spectroscopy of TOI-5205b Reveals Significant Stellar Contamination and a Metal-poor Atmosphere

  • Authors: Caleb I. Cañas, Jacob Lustig-Yaeger, Shang-Min Tsai, Simon Müller, Ravit Helled, Shubham Kanodia, Dana R. Louie, Giannina Guzmán Caloca, Peter Gao, Jessica Libby-Roberts, Kevin K. Hardegree-Ullman, Knicole D. Colón, Ian Czekala, Megan Delamer, Te Han, Andrea S.J. Lin, Suvrath Mahadevan, Erin M. May, Joe P. Ninan, Anjali A. A. Piette, Guðmundur Stefánsson, Kevin B. Stevenson, Johanna Teske, Nicole L. Wallack

Caleb I. Cañas et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 19.

Volume mixing ratios for select molecules, assuming chemical equilibrium and a clear atmosphere, obtained from POSEIDON (solid lines) when fitting the coadded spectrum. The shaded regions indicate the ±1σ−2σ model posteriors. The dashed lines are the abundances for H2O, CH4, CO, and H2S from the best-fitting VULCAN model in Table 3. From the forward model, these molecules are expected with VMRs <10−4 in stark contrast to the POSEIDON values where some trace molecules are found with VMRs > 0.01.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse