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Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations

  • Authors: Laura Sommovigo, Deaglan J. Bartlett, Rachel K. Cochrane, Matthew Ho, Christopher C. Lovell, Rachel S. Somerville

Laura Sommovigo et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 4.

Pareto front (equations minimizing RMSE for a given model length) of solutions found with OPERON for (left) the outer part of the attenuation curve, ﹩{\mathrm{log}}_{10}(f(x))﹩, and (right) the bump region of the attenuation curve, g(x). On the top, we plot the root mean-squared error (RMSE) on the target variable, and on the bottom, we plot the corresponding median absolute fractional error on the corresponding flux, ΔF/F. We plot the training and validation sets separately, and the vertical lines indicate our chosen models.

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