Simulation-based inference of galaxy properties from JWST pixels
The spectral energy distributions (SEDs) of galaxies offer detailed insights into their stellar populations, capturing key physical properties such as stellar mass, star formation history (SFH), metallicity, and dust attenuation. However, inferring these properties from SEDs is a highly degenerate inverse problem, particularly when using integrated
Iglesias-Navarro P. et al.
Fecha de publicación:
11
2025
Bibcode