A Survey of Model Fits to Brown Dwarf Spectra Through the L–T Sequence

We fit archival near-IR spectra of ∼300 brown dwarfs with atmosphere models from the Sonora and Phoenix groups. Using the parameters of the best-fit models as estimates for the physical properties of the brown dwarfs in our sample, we have performed a survey of how brown dwarf atmospheres evolve wit...

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Bibliographic Details
Main Authors: Savanah K. Turner, Denise C. Stephens, Conner B. Scoresby, Josh A. Miller
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astronomical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-3881/adda2a
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