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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 8.

Goodness of fit for the parameter space (atmospheric metallicity, haze monomer production rate, eddy diffusion coefficient, and haze optical properties) explored using the haze models. Note that the haze microphysical simulation failed to converge for cases with a haze monomer production rate of 10−10 g cm−2 s−1 in the 1× and 10× solar-metallicity cases due to the extremely high monomer production rate.

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