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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 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.
© 2026. The Author(s). Published by the American Astronomical Society.