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Using High-Resolution Spectroscopy to Study the Composition, Temperature, and Dynamics of Exoplanet Atmospheres

High-resolution spectroscopy, typically operating at resolving powers R greater or equal to 25,000, has matured into one of the primary techniques for characterising the atmospheres of extrasolar planets. The ability of HRS to resolve individual rotational-vibrational lines of molecular bands, combined with the large Doppler shifts experienced by close-
openaire   +1 more source

Nonthermal Atmospheric Losses for the Exoplanet GJ 3470b

Astronomy Reports, 2023
Valery Shematovich
exaly  

Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM

Nature, 2023
Björn Benneke   +2 more
exaly  

Phosphine as a Biosignature Gas in Exoplanet Atmospheres

Astrobiology, 2020
William Bains   +2 more
exaly  

Impact of photochemical hazes and gases on exoplanet atmospheric thermal structure

Monthly Notices of the Royal Astronomical Society, 2021
Panayotis Lavvas
exaly  

A Catalog of Exoplanet Atmospheric Retrieval Codes

Research Notes of the AAS, 2023
Natasha Batalha, Ryan J Macdonald
exaly  

Exploring and Validating Exoplanet Atmospheric Retrievals with Solar System Analog Observations

Planetary Science Journal, 2023
Arnaud Salvador, Tyler Robinson
exaly  

The science of ARIEL (Atmospheric Remote-sensing Infrared Exoplanet Large-survey)

Proceedings of SPIE, 2016
Neil Bowles   +2 more
exaly  

Atomic iron and titanium in the atmosphere of the exoplanet KELT-9b

Nature, 2018
Aurélien Wyttenbach   +2 more
exaly  

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