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. 2023 Jan 9;614(7949):670–675. doi: 10.1038/s41586-022-05674-1

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© The Author(s) 2023

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.

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Extended Data Fig. 8 — We fit for the K/O ratio while keeping the rest of the model parameters (for example, C/O ratio, metallicity and redistribution) the same as our reference model and fitting for the cloud parameters and scaled planetary radius. Here we present the different K/O ratio models (solid lines) we fit against the transmission spectrum at R = 300 (black and white points). We represent the respective fit of each model in the orange shading. (https://github.com/afeinstein20/wasp39b_niriss_paper/blob/main/scripts/edfigure8.py).