How do wavelength correlations affect transmission spectra? Application of a new fast and flexible 2D Gaussian process framework to transiting exoplanet spectroscopy

Open Access

Fig. L.6

Corner plot for 600RI data for analogous 2D GP fit (from Sect. 4.4.1). The wavelength-dependent parameters included are from the light curves centred on the Na and K features. We note that both the wavelength length scales $l_{λ_{C M}}$ $\[l_{\lambda_{\mathrm{CM}}}\]$ and $l_{λ_{H F S}}$ $\[l_{\lambda_{\mathrm{HFS}}}\]$ are constrained within the prior bounds for this dataset.

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