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. 2023 May 31;620(7973):292–298. doi: 10.1038/s41586-023-06230-1

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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. 3 — Comparison of the brightness temperature spectra obtained by fitting with ExoTEP the four separate reductions and binned at a resolving power of R = 50. All data are plotted with their 1σ error bars. We overplot the best-fit SCARLET model (blue line) to the reductions for further comparison. All reductions are consistent within less than one standard deviation on average when compared at full resolution (408 bins).

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