Fig. 3
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Example of the publicly available1 output data products for the planet TOI-3235 b (simulated with sunbather; Linssen et al. 2024). Left column: upper atmospheric structure. Right column: zoom-in on various parts of the transmission spectrum. The full spectrum spans 911 Å to 11 000 Å at a spectral resolution of R ~ 400 000. It includes spectral lines from the 30 lightest elements (up until zinc).
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