Ngā tūemi rite

• Charting the main sequence of star-forming galaxies out to redshifts z<5.7
  mā: Koprowski, M. P., me ētahi atu.
  I whakaputaina: (2024)
• Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z~6
  mā: Koprowski, M. P., me ētahi atu.
  I whakaputaina: (2025)
• The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
  mā: Cullen, F., me ētahi atu.
  I whakaputaina: (2023)
• No evidence (yet) for increased star-formation efficiency at early times
  mā: Donnan, C. T., me ētahi atu.
  I whakaputaina: (2025)
• JWST PRIMER: strong evidence for the environmental quenching of low-mass galaxies out to $\mathbf{\textit{z} \simeq 2}$
  mā: Hamadouche, M. L., me ētahi atu.
  I whakaputaina: (2024)