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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 16.
Absolute difference in BIC between spectral fits performed with and without an additional reddening/extinction term, using the Sonora Diamondback (top) and SM08 (bottom) atmospheric models, shown as a function of spectral type. Objects are shown in yellow where spectral fits including the extinction term are statistically preferred (i.e., BICNo Extinction − BICExtinction > 6), in green where fits excluding the extinction term are strongly preferred (i.e., BICNo Extinction − BICExtinction < −6), and in black where no statistically significant preference is found (∣BICNo Extinction − BICExtinction∣ < 6).
© 2026. The Author(s). Published by the American Astronomical Society.