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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 7.

Spectrum models for the three best-fit cases. The right vertical axis indicates the corresponding pressure levels for the best-fit model (blue line), which assumes a metallicity of 1× solar, a monomer production rate of ﹩\dot{M}=1{0}^{-13}﹩ g cm−2 s−1, an eddy diffusion coefficient of Kzz = 109 cm2 s−1, and soot optical properties.

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