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JWST COMPASS: NIRSpec/G395H Transmission Observations of the Sub-Neptune HD 15337 c

  • Authors: Nicole L. Wallack, Peter Gao, Michael Greklek-McKeon, Annabella Meech, Artyom Aguichine, Munazza K. Alam, Lili Alderson, Natasha E. Batalha, Natalie M. Batalha, Anna Gagnebin, Tyler A. Gordon, James Kirk, Mercedes López-Morales, Sarah E. Moran, Jea Iyanla Redai, Nicholas Scarsdale, Johanna Teske, Hannah R. Wakeford, Nicholas F. Wogan, Angie Wolfgang

Nicole L. Wallack et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 13.

σ-rejection contours in metallicity–opaque pressure level (Popaque) space from our PLATON retrievals for Eureka! (top) and Tiberius (bottom) reductions of the combined (left), visit 1 (middle), and visit 2 (right) data. The 1σ, 2σ, and 3σ contours in 2D are indicated. The mean molecular weight at 1 bar in an isothermal atmosphere with HD 15337 c’s equilibrium temperature is shown on the top axes and corresponds to the metallicities on the bottom axes, computed using PLATON assuming C/O = 0.59 and thermochemical equilibrium. Minimum allowed clear-atmosphere metallicities for the more constraining datasets are indicated by the vertical dashed lines, while the maximum allowed Popaque values at lower metallicities are indicated by the horizontal dotted lines.

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