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Thermal structure, composition, atmospheric dynamics and long-terme evolution of irradiated exoplanets

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Academic year: 2021

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Figure 1. Number of known planets as a function of time listed by detection technique.
Figure 1.5. Toy model simulations of  ground-based spectra of hot Jupiters as a function of planet orbital phase, targeting carbon monoxide (left) and methane (right).
Table 1.2. Claimed detections of sodium in exoplanets’ atmospheres from transit spec- spec-trophotometry.
Table 1.3. Claimed detections of potassium in exoplanets’ atmospheres from transit spec- spec-trophotometry.
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