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- W3103133674 abstract "We present high-resolution optical transmission spectroscopy of two sub-Saturn mass transiting exoplanets, HAT-P-12b and WASP-69b. With relatively low densities and high atmospheric scale heights, these planets are particularly well-suited to characterization through transit spectroscopy, and serve as ideal candidates for extending previously tested methods to lower planetary masses. Using a single transit for each planet, we take advantage of the Doppler cross-correlation technique to search for sodium, potassium, and water absorption features. Our analysis reveals a likely (3.2σ) detection of sodium absorption features in the atmosphere of HAT-P-12b, and enables us to place constraints on the presence of alkaline and molecular species in the atmospheres of both planets. With our results, we highlight the efficacy of ground-based campaigns for characterizing exoplanetary atmospheres and pave the way for future analyses of low-mass planets." @default.
- W3103133674 created "2020-11-23" @default.
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- W3103133674 date "2019-01-18" @default.
- W3103133674 modified "2023-10-01" @default.
- W3103133674 title "High-resolution Transit Spectroscopy of Warm Saturns" @default.
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- W3103133674 doi "https://doi.org/10.3847/1538-3881/aaf56b" @default.
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