Galaxy luminosity functions from far-UV to submillimetre at $z=0$ in the COLIBRE simulations

Documenti analoghi

• The galaxy ultraviolet luminosity function from $z=7$ to $15$ in the COLIBRE simulations
  di: Lu, Shengdong, et al.
  Pubblicazione: (2026)
• Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
  di: Benítez-Llambay, Alejandro, et al.
  Pubblicazione: (2025)
• The evolution of the galaxy stellar mass function and star formation rates in the COLIBRE simulations from redshift 17 to 0
  di: Chaikin, Evgenii, et al.
  Pubblicazione: (2025)
• The morphologies of present-day galaxies in the COLIBRE simulations
  di: Moreno, Victor J. Forouhar, et al.
  Pubblicazione: (2026)
• A hybrid active galactic nucleus feedback model with spinning black holes, winds and jets
  di: Huško, Filip, et al.
  Pubblicazione: (2025)