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GEMS JWST: HATS-75 b A Giant Planet with a Subsolar Metallicity Atmosphere Orbiting an M Dwarf

  • Authors: Reza Ashtari, Jacob Lustig-Yaeger, Jessica Libby-Roberts, Simon Müller, Shubham Kanodia, Kevin B. Stevenson, Caleb I. Cañas, Giannina Guzmán Caloca, Nicole L. Wallack, Megan Delamer, Anjali A. A. Piette, Suvrath Mahadevan, Ian Czekala, Te Han, Ravit Helled

Reza Ashtari et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 2.

Modeled fleck star spots for Visits 1 (top) and 2 (bottom). Visit 3 is not shown because the preferred transit model is spot-free for the Eureka!+fleck reduction. Interestingly, the spots share roughly the same latitude across the transit chord, with similar spot contrasts of 0.960 ± 0.008 and 0.971 ± 0.002 for Visits 1 and 2, respectively. Characteristics for the spots modeled for both reductions are detailed in Table A1.

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