Atmospheric characterisation and tighter constraints on the orbital misalignment of WASP-94 A b with HARPS
arxiv(2024)
摘要
We present high spectral resolution observations of the hot Jupiter WASP-94 A
b using the HARPS instrument on ESO's 3.6m 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.
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