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A JWST Transiting Survey of FGK Stellar Limb Darkening: Empirical Evidence for Quadratic Laws and Atmospheric Model Comparisons

  • Authors: David K. Sing, Joshua D. Lothringer, Jeff A. Valenti, Natalie H. Allen, Katherine A. Bennett, Carlos Gascón, Mei Ting Mak, Patrick McCreery, Sagnick Mukherjee, Lakeisha M. Ramos Rosado, Stephen P. Schmidt, Kevin B. Stevenson, Daniel P. Thorngren, Le-Chris Wang

David K. Sing et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 8.

(Top) Same as Figure 6, but for WASP-6 using the MURaM magnetic models: with small-scale turbulent dynamo (SSD) baseline model (blue) and B-fields of 100 G, 200 G, and 300 G (orange, greed, purple respectively) shown. The change in LD parameters ℓ (middle) and δ (bottom) between the nonmagnetic model and model with B-fields is also shown.

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