Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
Cosmological hydrodynamical simulations provide valuable insights on galaxy evolution when coupled with observational data. Comparisons with real galaxies are typically performed via scaling relations of the observables. Here, we follow an alternative approach based on the spectral covariance in a model-independent way. We build upon previous work
Sharbaf, Z. et al.
Fecha de publicación:
5
2025