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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 6.

Comparison of spectroscopically inferred Teff, ﹩\mathrm{log}(g)﹩, fsed, and R values between Sonora Diamondback and SM08 model grids. Uncertainties in Teff, ﹩\mathrm{log}(g)﹩, and fsed are adopted as half the model grid spacing and are not plotted for clarity. Model grids are indicated by gray dashed lines. In the ﹩\mathrm{log}(g)﹩ and fsed panels, data points are clustered at discrete grid values; the number of targets at each value is labeled.

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