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Are there Spectral Features in the MIRI/LRS Transmission Spectrum of K2-18b?

2025/04/22 by Jake Taylor, Taylor, Jake · 11 voices · 5 citations
Engineering · #Particle Accelerators and Free-Electron Lasers #Astronomical Observations and Instrumentation #Particle accelerators and beam dynamics

paper · pdf · doi:10.48550/arxiv.2504.15916

Abstract

Determining the composition of an exoplanet atmosphere relies on the presence of detectable spectral features. The strongest spectral features, including DMS, look approximately Gaussian. Here, I perform a suite of Gaussian feature analyses to find any statistically significant spectral features in the recently published MIRI/LRS spectrum of K2-18b (N. Madhusudhan et al. 2025). In N. Madhusudhan et al. 2025, they claim a 3.4-σ detection of spectral features compared to a flat line. In 5 out of 6 tests, I find the data preferred a flat line over a Gaussian model, with a χ2ν of 1.06. When centering the Gaussian where the absorptions for DMS and DMDS peak, I find ln(B) = 1.21 in favour of the Gaussian model, with a χ2ν of 0.99. With only ∼2-σ in favour of Gaussian features, I conclude no strong statistical evidence for spectral features.

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