Ngā tūemi rite

• Semi-analytic modelling of Pop. III star formation and metallicity evolution -- I. Impact on the UV luminosity functions at z = 9-16
  mā: Ventura, Emanuele M., me ētahi atu.
  I whakaputaina: (2024)
• Uncovering the physical origin of the prominent Lyman-$α$ emission and absorption in GS9422 at $z = 5.943$
  mā: Terp, Chamilla, me ētahi atu.
  I whakaputaina: (2024)
• Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum
  mā: Ventura, Emanuele M., me ētahi atu.
  I whakaputaina: (2025)
• MOSEL survey: Spatially offset Lyman-continuum emission in a new emitter at z=3.088
  mā: Gupta, Anshu, me ētahi atu.
  I whakaputaina: (2024)
• Cosmic Reionization On Computers: Statistics, Physical Properties and Environment of Lyman Limit Systems at $z\sim6$
  mā: Fan, Jiawen, me ētahi atu.
  I whakaputaina: (2022)