Reliability of 1D radiative-convective photochemical-equilibrium retrievals on transit spectra of WASP-107b
arXiv:2508.00177 · doi:10.1051/0004-6361/202554885
Abstract
Observations of WASP-107b suggest a metal-rich and carbon-deprived atmosphere with an extremely hot interior based on detections of SO, HO, CO, CO, NH, and CH. In this paper, we aim to determine the reliability of a 1D radiative-convective photochemical-equilibrium (1D-RCPE) retrieval method in inferring atmospheric properties of WASP-107b. Our grid of radiative-convective balanced pressure-temperature profiles and 1D photochemical equilibrated models covers a range of metallicities (Z), carbon-to-oxygen ratios (C/O), intrinsic temperatures (T), and eddy diffusion coefficients (K). We obtain good fits with our 1D-RCPE retrievals based on a few molecular features of HO, CO, SO, and CH, but find no substantial contribution of NH. We find that the degeneracy between metallicity, cloud pressure, and a model offset is broken by the presence of strong SO features, confirming that SO is a robust metallicity indicator. We systematically retrieve sub-solar C/O based on the relative amplitude of a strong CO feature with respect to the broad band of HO, which is sensitive to a wavelength-dependent scattering slope. We find that high-altitude clouds obscure the CH-rich layers, preventing the retrievals from constraining T, but that higher values of K can transport material above the cloud deck, allowing a fit of the CH feature. However, T and K can vary substantially between retrievals depending on the adopted cloud parametrization. We conclude that the 1D-RCPE retrieval method can provide useful insights if the underlying grid of forward models is well understood. We find that WASP-107b's atmosphere is enriched in metals (3 to 5 times solar) and carbon-deprived (C/O <= 0.20). However, we lack robust constraints on the intrinsic temperature and vertical mixing strength.
30 pages, 18 figures, 5 tables, accepted by A&A
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