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How accurately can obscured galaxy luminosities be measured using spectral energy distribution fitting of near- through far-infrared observations?

Fuente: arXiv

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Bibliographic Details
Main Authors:	Farrah, Duncan, Ejercito, Kiana, Efstathiou, Andreas, Leisawitz, David, Engholm, Athena, Shivaei, Irene, Bonato, Matteo, Clements, David L., Petty, Sara, Pitchford, Lura. K., Varnava, Charalambia, Afonso, Jose, Gruppioni, Carlotta, Hatziminaoglou, Evanthia, Hoffman, Andrew, Lacy, Mark, Matthews, Brenda C., Nixon, Conor, Pearson, Chris, Ricketti, Berke Vow, Rigopoulou, Dimitra, Robinson, Loren, Spencer, Locke D., Wang, Lingyu, Sanders, David B., van Belle, Gerard
Format:	Preprint
Published:	2025
Subjects:	Astrophysics of Galaxies
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2511.13849