Angelos Nersesian

2 та иш

STAR Institute, Université de Liège

1. Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions

   Kosei Matsumoto, Laura Sommovigo, Andrea Gebek +8

   МақолаGalaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysics20250 иқтибос

   ABIABI:AkademIndex/openalex/2025.article.001474

2. <i>Euclid</i> preparation

   Angelos Nersesian, Abdurro’uf, M. Baes +97

   МақолаGalaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysics20250 иқтибос

   ABIABI:AkademIndex/openalex/2025.article.002636