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Uniform Forward-modeling Analysis of Ultracool Dwarfs. IV. Benchmarking the Sonora Diamondback and D. Saumon & M. S. Marley (2008) Atmospheric Models Across Late M, L, and T Types with Low-resolution 0.8–2.5 μm Spectroscopy
Emily Mader et al 2026 The Astronomical Journal 171 .
Caption: Figure 8.
Cumulative distributions (solid lines) of the best-fit fsed values inferred from the Sonora Diamondback models for benchmark brown dwarfs in the L0–T5 (top left), L0–L9 (top middle), T0–T5 (top right), and L4–L9 (bottom) type ranges. Young (<300 Myr) and old (≤300 Myr) benchmarks are shown in blue and orange, respectively. The corresponding normalized histograms of the fsed distributions are overlaid.
© 2026. The Author(s). Published by the American Astronomical Society.