A 100 Mpc$^2$ structure traced by hyperluminous galaxies around a massive $z$ = 2.85 protocluster

Documenti analoghi

• Kinematic analysis of $\mathbf{z = 4.3}$ galaxies in the SPT2349$-$56 protocluster core
  di: Venkateshwaran, Aparna, et al.
  Pubblicazione: (2024)
• Evidence for environmental effects in the $z\,{=}\,4.3$ protocluster core SPT2349$-$56
  di: Hughes, Chayce, et al.
  Pubblicazione: (2024)
• Improving Optical Photo-z Constraints for Dusty Star-forming Galaxies Using Submillimeter-based Priors
  di: Tanouri, Pouya, et al.
  Pubblicazione: (2024)
• Modelling the multi-wavelength detection of protoclusters. I: An excess of submillimetre galaxies in protocluster cores
  di: Araya-Araya, Pablo, et al.
  Pubblicazione: (2024)
• An ALMA spectroscopic survey of the Planck high-redshift object PLCK G073.4-57.5 confirms two protoclusters
  di: Hill, Ryley, et al.
  Pubblicazione: (2024)