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Atmospheric characterization and tighter constraints on the orbital misalignment of WASP-94 A b with HARPS
Ahrer, E.
Seidel, J.
Doyle, L.
Gandhi, S.
Prinoth, B.
Cegla, H.
McDonald, C.
Ayache, E.
Nealon, R.
Veras, Dimitri
Wheatley, P.
Ehrenreich, D.
Oxford Academic
2024
We present high spectral resolution observations of the hot Jupiter WASP-94 A b using the HARPS instrument on ESO’s 3.6-m telescope in La Silla, Chile. We probed for Na absorption in its atmosphere as well as constrained the previously reported misaligned retrograde orbit using the Rossiter–McLaughlin effect. Additionally, we undertook a combined atmospheric retrieval analysis with previously published low-resolution data. We confirm the retrograde orbit as well as constrain the orbital misalignment with our measurement of a projected spin-orbit obliquity of λ = 123.0 ± 3.0°. We find a tentative detection of Na absorption in the atmosphere of WASP-94 A b, independent of the treatment of the Rossiter–McLaughlin effect in our analysis (3.6σ and 4.4σ). We combine our HARPS high-resolution data with low-resolution data from the literature and find that while the posterior distribution of the Na abundance results in a tighter constraint than using a single data set, the detection significance does not improve (3.2σ), which we attribute to degeneracies between the low- and high-resolution data.
Name
Atmospheric characterization and tighter constraints on the orbital misalignment of WASP-94 A b with HARPS.pdf
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8.32 MB
Format
Checksum
observ ational
spectroscopic
Exoplanets
atmospheres
WASP-94 A b.