Going Wide and Deep with Roman: The z~6-9 UV luminosity function in a Roman Deep Field

Ejemplares similares

• Faint active galactic nuclei supplied 31-75% of hydrogen-ionizing photons at z>5
  por: Singha, Mainak, et al.
  Publicado: (2025)
• The BoRG-$JWST$ Survey: Analogs at $z\sim8$ to the UV-luminous Galaxy Population at $z\gtrsim10$
  por: Rojas-Ruiz, Sofía, et al.
  Publicado: (2025)
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
  por: Somerville, Rachel S., et al.
  Publicado: (2025)
• Evolution of H$α$ Equivalent Widths from $z \sim 0.4-2.2$: implications for star formation and legacy surveys with Roman and Euclid
  por: Khostovan, Ali Ahmad, et al.
  Publicado: (2024)
• ESpRESSO -- Forward modeling Roman Space Telescope spectroscopy
  por: Gabrielpillai, Austen, et al.
  Publicado: (2024)