Ngā tūemi rite

• JWST ASPIRE: How Did Galaxies Complete Reionization? Evidence for Excess IGM Transmission around ${\rm [O\,{\scriptstyle III}]}$ Emitters during Reionization
  mā: Kakiichi, Koki, me ētahi atu.
  I whakaputaina: (2025)
• A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at $z=4-6$
  mā: Sun, Fengwu, me ētahi atu.
  I whakaputaina: (2024)
• A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Broad-line AGN at $z=4-5$ revealed by JWST/NIRCam WFSS
  mā: Lin, Xiaojing, me ētahi atu.
  I whakaputaina: (2024)
• A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Impact of Galaxies on the CGM Metal Enrichment at z > 6 Using the JWST and VLT
  mā: Zou, Siwei, me ētahi atu.
  I whakaputaina: (2024)
• ASPIRE: The Environments and Dark Matter Halos of Luminous Quasars in the Epoch of Reionization
  mā: Wang, Feige, me ētahi atu.
  I whakaputaina: (2026)