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The James Webb Space Telescope NIRSpec-PRISM Transmission Spectrum of the Super-puff, Kepler-51d

  • Authors: Jessica E. Libby-Roberts, Aaron Bello-Arufe, Zachory K. Berta-Thompson, Caleb I. Cañas, Yayaati Chachan, Renyu Hu, Yui Kawashima, Catriona Murray, Kazumasa Ohno, Armen Tokadjian, Suvrath Mahadevan, Kento Masuda, Leslie Hebb, Caroline Morley, Guangwei Fu, Peter Gao, Kevin B. Stevenson

Jessica E. Libby-Roberts et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 1.

Top panel: the best-fit spotrod and starry spot configurations represented on Kepler-51. Middle panel: the JWST white light curve of Kepler-51d with flux binned from 0.6–5.3 μm. Points are binned to 30 s for clarity. Best-fit models from the above spotrod and starry are plotted in orange and blue, respectively. Regardless of the spot configuration, the white light-curve models are identical. Bottom panel: plot showcasing the white light-curve residuals from the spotrod best-fit model above.

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