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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 16.

Top: a comparison of published ARCTIC photometry from S. Kanodia et al. (2023) with the photometry derived in this work. Bottom: a zoom into the region indicated by a rectangle on the top panel. Both panels display the phase-folded photometry for ARCTIC transits from S. Kanodia et al. (2023), the TESS data derived using a point-spread function to attempt to correct for dilution, and the JWST data. All ARCTIC transits and all TESS transits (before and after JWST observations) are deeper than the white light curves from JWST.

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