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Evidence of Water Vapor in the Atmosphere of a Metal-Rich Hot Saturn with High-Resolution Transmission Spectroscopy

1 Jul 2024arXiv:2407.01266links table onlyarchive 2025-07-28

Sayyed A. Rafi, Stevanus K. Nugroho, Motohide Tamura, Lisa Nortmann, Alejandro Sánchez-López

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Transmission spectroscopy presents one of the most successful approaches for investigating the atmospheres of exoplanets. We analyzed the near-infrared high-resolution transmission spectrum of a hot Saturn, HD 149026 b, taken using CARMENES spectrograph (ℛ∼80,400). We found evidence of H₂O at an S/N of ∼4.8. We also performed grid search using a Bayesian framework and constrained the orbital velocity Kₚ and rest velocity Vᵣₑₛₜ to 158.17^(+8.31)_(-7.90) km s⁻¹ and 2.57^(+0.54)_(-0.57) km s⁻¹, respectively. Whilst the retrieved Kₚ value is consistent with theoretical prediction, the retrieved Vᵣₑₛₜ value is highly red-shifted ($>3-\sigma$). This might be an indication of either anomalous atmospheric dynamics at play or an orbit with non-zero eccentricity. Additionally, we searched for HCN but no successful detection has been made possibly due to the relatively low S/N dataset. The detection of H₂O and subsequent abundance retrieval, coupled with analysis of other species such as CO at the K-band, for example, might help us to get some information about the atmospheric C/O ratio and metallicity, which in turn could give us some insight into the planet formation scenario.

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