On Atmospheric Retrievals of Exoplanets with Inhomogeneous Terminators
Luis Welbanks, Nikku Madhusudhan

TL;DR
This study evaluates the limitations of 1D atmospheric models in exoplanet transmission spectra retrievals, demonstrating that biases are often due to model assumptions rather than inherent model constraints, and introduces a 2D retrieval framework for improved analysis.
Contribution
The paper systematically assesses 1D model biases and introduces a 2D retrieval framework to better account for atmospheric inhomogeneities in exoplanet spectra.
Findings
Biases in 1D retrievals often stem from model assumptions.
Revised temperature estimates for WASP-43b and WASP-103b align with expectations.
A 2D retrieval method improves constraints on atmospheric properties.
Abstract
The complexity of atmospheric retrieval models is largely data-driven and one-dimensional models have generally been considered adequate with current data quality. However, recent studies have suggested that using 1D models in retrievals can result in anomalously cool terminator temperatures and biased abundance estimates even with existing transmission spectra of hot Jupiters. Motivated by these claims and upcoming high-quality transmission spectra we systematically explore the limitations of 1D models using synthetic and current observations. We use 1D models of varying complexity, both analytic and numerical, to revisit claims of biases when interpreting transmission spectra of hot Jupiters with inhomogeneous terminator compositions. Overall, we find the reported biases to be resulting from specific model assumptions rather than intrinsic limitations of 1D atmospheric models in…
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