Discriminating between hazy and clear hot-Jupiter atmospheres with CARMENES
            
    Context. Relatively large radii of some hot Jupiters observed in the ultraviolet and blue-optical are generally interpreted to be due to Rayleigh scattering by high-altitude haze particles. However, the haze composition and its production mechanisms are not fully understood, and observational information is still limited. Aims: We aim to study the
            Sánchez-López, A. et al.
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                        2020