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C, N, O, S, and Photochemistry in a Temperate Giant Planet Orbiting a Late M Dwarf

  • Authors: Michael Zhang, Qiao Xue, Jeehyun Yang, Vighnesh Nagpal, Michael R. Line, Guangwei Fu, Matthew C. Nixon, Jacob L. Bean, Peter Gao, Eliza M.-R. Kempton, Luis Welbanks, Edward M. Bryant, Daniel Bayliss, Madison Brady, Jean-Michel Désert, Vincent Van Eylen, Jonathan J. Fortney, Andrés Jordán, Vivien Parmentier, Caroline Piaulet-Ghorayeb, Elyar Sedaghati, Kevin B. Stevenson, Amaury H. M. J. Triaud

Michael Zhang et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 1.

The normalized, uncorrected white light curve of TOI-6894 b spanning 0.8–5.2 μm, with the best-fit transit model overplotted in red. The first 500 integrations are discarded to get rid of detector settling effects. The vertical dashed lines indicate the times of ingress and egress. Binned residuals are shown below with the y-axis magnified by a factor of 76 relative to the upper panel.

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