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JWST TRAPPIST-1 e/b Program: Motivation and First Observations

Authors: Natalie H. Allen, Néstor Espinoza, V. A. Boehm, Caleb I. Cañas, Kevin B. Stevenson, Nikole K. Lewis, Ryan J. MacDonald, Brett M. Morris, Eric Agol, Knicole Colón, Hannah Diamond-Lowe, Ana Glidden, Amélie Gressier, Jingcheng Huang, Zifan Lin, Douglas Long, Dana R. Louie, Meredith A. MacGregor, Laurent Pueyo, Benjamin V. Rackham, Sukrit Ranjan, Sara Seager, Guadalupe Tovar Mendoza, Jeff A. Valenti, Daniel Valentine, Roeland P. van der Marel, Hannah R. Wakeford

Natalie H. Allen et al 2026 The Astronomical Journal 171 .

Provider: AAS Journals

Caption: Figure 10.

Same as Figure 4, but in absolute spectrum ratio. The dashed lines of each color represent the median spectrum ratio for each reduction. Observation 15 shows an offset in absolute spectrum ratio depth due to the difference of treatment of flares, which can also be seen in the individual TRAPPIST-1 e spectrum in Figure 9.

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