The Steep-spectrum Radio-loud AGN Luminosity Function and Its Implications for Black Hole Growth and Star Formation

Documenti analoghi

• Revisiting the 150 MHz Radio Luminosity Function of Star-Forming Galaxies with LOFAR Deep Fields through a Refined Statistical Framework
  di: Wang, Wenjie, et al.
  Pubblicazione: (2025)
• Constraints on cosmic star formation history via a new modeling of the radio luminosity function of star-forming galaxies
  di: Wang, Wenjie, et al.
  Pubblicazione: (2023)
• Decomposing Infrared Luminosity Functions into Star-Forming and AGN Components using CIGALE
  di: Lyon, Daniel J., et al.
  Pubblicazione: (2024)
• The nature of compact radio-loud AGN: a systematic look at the LOFAR AGN population
  di: Chilufya, J., et al.
  Pubblicazione: (2024)
• A Steep Decline in the Galaxy Space Density Beyond Redshift 9 in the CANUCS UV Luminosity Function
  di: Willott, Chris J., et al.
  Pubblicazione: (2023)