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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 5.

Best-fit synthetic spectra for all targets using the SM08 models (blue) and Sonora Diamondback (red) models, overlaid with the observed IRTF/SpeX spectra (black). Fluxes within the broad water bands (shaded in gray) are masked in spectral fits. Targets are ordered by spectral types, spanning M7–T8.

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