Emulating radiative transfer with artificial neural networks

ABSTRACT Forward-modeling observables from galaxy simulations enables direct comparisons between theory and observations. To generate synthetic spectral energy distributions (SEDs) that include dust absorption, re-emission, and scattering, Monte Carlo radiative transfer is often used in post-process...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2023-10, Vol.526 (3), p.4520-4528
Hauptverfasser:	Sethuram, Snigdaa S, Cochrane, Rachel K, Hayward, Christopher C, Acquaviva, Viviana, Villaescusa-Navarro, Francisco, Popping, Gergö, Wise, John H
Format:	Artikel
Sprache:	eng
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