Broadband transmission spectroscopy of HD209458b with ESPRESSO: Evidence for Na, TiO, or both
N. C. Santos, E. Cristo, O. Demangeon, M. Oshagh, R. Allart, S. C. C., Barros, F. Borsa, V. Bourrier, N. Casasayas-Barris, D. Ehrenreich, J. P., Faria, P. Figueira, J. H. C. Martins, G. Micela, E. Pall\'e, A. Sozzetti, H., M. Tabernero, M. R. Zapatero Osorio, F. Pepe

TL;DR
This study uses high-resolution ESPRESSO spectra to analyze the atmosphere of exoplanet HD209458b, finding potential evidence for sodium, titanium oxide, or both, and demonstrating ground-based spectroscopy's capabilities.
Contribution
First application of the chromatic Rossiter-McLaughlin method with ESPRESSO to derive broadband transmission spectra of an exoplanet from ground-based data.
Findings
Transmission spectrum similar to HST observations
Possible presence of Na, TiO, or both in the atmosphere
Ground-based high-resolution spectroscopy is effective for exoplanet atmosphere studies
Abstract
The detection and characterization of exoplanet atmospheres is currently one of the main drivers pushing the development of new observing facilities. In this context, high-resolution spectrographs are {proving} their potential and showing that high-resolution spectroscopy will be paramount in this field. We aim to make use of ESPRESSO high-resolution spectra, which cover two transits of HD209458b, to probe the broadband transmission optical spectrum of the planet. We applied the chromatic Rossiter-McLaughin method to derive the transmission spectrum of HD209458b. We compared the results with previous HST observations and with synthetic spectra. We recover a transmission spectrum of HD209458b similar to the one obtained with HST data. The models suggest that the observed signal can be explained by only Na, only TiO, or both Na and TiO, even though none is fully capable of explaining our…
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