In 5 of 6 Gaussian feature tests, the K2-18b MIRI/LRS spectrum prefers a flat line over spectral features, with only weak evidence (ln(B)=1.21) for features at fixed wavelengths.
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Are there Spectral Features in the MIRI/LRS Transmission Spectrum of K2-18b?
In 5 of 6 Gaussian feature tests, the K2-18b MIRI/LRS spectrum prefers a flat line over spectral features, with only weak evidence (ln(B)=1.21) for features at fixed wavelengths.