Abstract
Ground-based high-resolution and space-based low-resolution spectroscopy
are the two main avenues through which transiting exoplanet atmospheres
are studied. Both methods provide unique strengths and shortcomings,
and combining the two can be a powerful probe into an exoplanet's
atmosphere. Within a joint atmospheric retrieval framework, we combined
JWST NIRSpec/G395H secondary eclipse spectra and Gemini South/IGRINS
pre- and post-eclipse thermal emission observations of the hot Jupiter
WASP-77A b. Our inferences from the IGRINS and NIRSpec data sets are
consistent with each other, and combining the two allows us to measure
the gas abundances of H2O and CO, as well as the vertical
thermal structure, with higher precision than either data set provided
individually.
Original language | English |
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Article number | 110 |
Journal | Astronomical Journal |
Volume | 167 |
Issue number | 3 |
Number of pages | 24 |
ISSN | 0004-6256 |
DOIs | |
Publication status | Published - 2024 |
Keywords
- Exoplanets
- Exoplanet astronomy
- Extrasolar gaseous planets
- Hot Jupiters
- Exoplanet atmospheres
- Exoplanet atmospheric composition
- Spectroscopy
- High resolution spectroscopy