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Photometric Variability and Rotation of β Pictoris b from JWST NIRCam Coronagraphic Imaging

  • Authors: Yifan Zhou, Beth A. Biller, Aarynn L. Carter, Marshall D. Perrin, Michael Poon, Genaro Suárez, Ben J. Sutlieff, Johanna M. Vos, Jason J. Wang, William O. Balmer, Marta L. Bryan, Anthony Boccaletti, Julien H. Girard, Eileen C. Gonzales, Jens Kammerer, Jarron M. Leisenring, Paulina. Palma-Bifani, Kevin R. Wagner, Dániel Apai, Mickäel Bonnefoy, Brendan P. Bowler, Kyle Franson, Pengyu Liu, Marcio Meléndez, Stanimir A. Metchev, Simon Petrus, Laurent Pueyo, Isabel Rebollido, Andrew J. Skemer, Xianyu Tan, Niall Whiteford

Yifan Zhou et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 6.

F210M and F410M light curves (the Fi(t) term in Equation (1)). Light curves measured in the planet apertures are plotted in black lines and the comparison aperture light curves are plotted in the same colors as their apertures in Figure 5.

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