A Comparative L-dwarf Sample Exploring the Interplay Between Atmospheric Assumptions and Data Properties
Eileen C. Gonzales, Ben Burningham, Jacqueline K. Faherty, Nikole K., Lewis, Channon Visscher, and Mark Marley

TL;DR
This study compares atmospheric retrievals of five L dwarfs to understand how metallicity and data quality influence atmospheric models, revealing that high SNR data limits are dominated by model uncertainties and highlighting methods to resolve cloud model degeneracies.
Contribution
It presents the first atmospheric retrievals for four L dwarfs, analyzing the effects of metallicity and SNR on atmospheric parameters, and discusses strategies to resolve cloud model degeneracies.
Findings
Similar Teff sources have comparable P-T profiles with metallicity affecting profile offsets.
At SNR ≥80, model uncertainties dominate over measurement errors.
SNR influences confidence in parameters but not the ability to distinguish cloud models.
Abstract
Comparisons of atmospheric retrievals can reveal powerful insights on the strengths and limitations of our data and modeling tools. In this paper, we examine a sample of 5 similar effective temperature (Teff) or spectral type L dwarfs to compare their pressure-temperature (P-T) profiles. Additionally, we explore the impact of an object's metallicity and the observations' signal-to-noise (SNR) on the parameters we can retrieve. We present the first atmospheric retrievals: 2MASS J152614052043414, 2MASS J053952000059019, 2MASS J153941890520428, and GD 165B increasing the small but growing number of L-dwarfs retrieved. When compared to atmospheric retrievals of SDSS J141624.08+134826.7, a low-metallicity d/sdL7 primary in a wide L+T binary, we find similar Teff sources have similar P-T profiles with metallicity differences impacting the relative offset between their P-T profiles in…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Meteorological Phenomena and Simulations · Statistical and numerical algorithms
