# LRG-BEASTS: transmission spectroscopy and retrieval analysis of the highly-inflated Saturn-mass planet WASP-39b

## TL;DR

This study presents a ground-based transmission spectrum and retrieval analysis of the exoplanet WASP-39b, revealing consistently high atmospheric metallicity and emphasizing the impact of retrieval assumptions on abundance estimates.

## Contribution

It provides a comprehensive retrieval analysis of all literature data for WASP-39b, demonstrating that retrieval assumptions significantly influence derived atmospheric metallicities.

## Key findings

- Retrieved highly supersolar metallicities across all data sets
- Combined spectrum analysis yields metallicity of approximately 282 times solar
- Stellar activity has negligible effect on abundance estimates

## Abstract

We present a ground-based transmission spectrum and comprehensive retrieval analysis of the highly inflated Saturn-mass planet WASP-39b. We obtained low-resolution spectra ($R \approx 400$) of a transit of WASP-39b using the ACAM instrument on the 4.2m William Herschel Telescope as part of the LRG-BEASTS survey. Our transmission spectrum is in good agreement with previous ground- and space-based observations of WASP-39b, and covers a wavelength range of 4000-9000A. Previous analyses of this exoplanet have retrieved water abundances that span more than four orders of magnitude, which in turn lead to conclusions of a subsolar or highly supersolar atmospheric metallicity. In order to determine the cause of the large discrepancies in the literature regarding WASP-39b's atmospheric metallicity, we performed retrieval analyses of all literature data sets. Our retrievals, which assume equilibrium chemistry, recovered highly supersolar metallicities for all data sets. When running our retrievals on a combined spectrum, spanning 0.3-5$\mu$m, we recovered an atmospheric metallicity of $282^{+65}_{-58} \times$ solar. We find that stellar activity has a negligible effect on the derived abundances and instead conclude that different assumptions made during retrieval analyses lead to the reported water abundances that differ by orders of magnitude. This in turn has significant consequences for the conclusions we draw. This is the fourth planet to be observed as part of the LRG-BEASTS survey, which is demonstrating that 4m class telescopes can obtain low-resolution transmission spectra with precisions of around one atmospheric scale height.