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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

  • Authors: Emily Mader, Zhoujian Zhang, 周健 张, Jonathan J. Fortney, Caroline V. Morley, Malik Bossett, Mark S. Marley, Sagnick Mukherjee, Brendan P. Bowler, Michael C. Liu

Emily Mader et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

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.

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