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Muted Features in the JWST NIRISS Transmission Spectrum of Hot Neptune LTT 9779b

  • Authors: Michael Radica, Louis-Philippe Coulombe, Jake Taylor, Loic Albert, Romain Allart, Björn Benneke, Nicolas B. Cowan, Lisa Dang, David Lafrenière, Daniel Thorngren, Étienne Artigau, René Doyon, Laura Flagg, Doug Johnstone, Stefan Pelletier, Pierre-Alexis Roy

Michael Radica et al 2024 The Astrophysical Journal Letters 962 .

  • Provider: AAS Journals

Caption: Figure 1.

The population of close-in exoplanets visualized in period–radius space. All confirmed planets (from the NASA Exoplanet Archive), with masses and radii measured to better than 15% and 10%, respectively, are shown colored by the amount of flux they receive from their host star relative to the Earth. The hot Neptune desert, as defined by Mazeh et al. (2016), is marked in gray, and LTT 9779 b is identified with a star.

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