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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 4.

χ2-based spectral fitting results of three representative targets based on the Sonora Diamondback atmospheric models. In the left panels, the observed IRTF/SpeX spectra (black) are compared with the best-fit model spectra (red), and the corresponding best-fit parameters are labeled. Fluxes within the broad water bands (shaded in gray) are masked in spectral fits. The right panels present the χ2 values as a function of effective temperatures, with variations in symbol, color, and transparency indicating different values of ﹩\mathrm{log}(g)﹩, fsed, and [M/H], respectively.

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