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Retrieving temperatures and abundances of exoplanet atmospheres with high resolution cross correlation spectroscopy

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Figure

Figure 1. Illustration of the key components of the HRCCS retrieval algorithm.Many components are the same as in a classic “low-resolution” retrieval: theforward model, the data, and the Bayesian estimator
Table 1
Table 2
Figure 4. Retrieved constraints from the simulated HDS data set. Constraints are summarized with a corner diagram for the abundances and velocities, and thein the remainder of the manuscript were generated with a modiratiotoproon the retrieved scale factor
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