An X-ray-Emitting Proto-Cluster at $z\approx5.7$ Reveals Rapid Structure Growth

Documenti analoghi

• Chandra Rules Out Super-Eddington Accretion Models For Little Red Dots
  di: Sacchi, Andrea, et al.
  Pubblicazione: (2025)
• The Massive and Distant Clusters of $WISE$ Survey. XII. Exploring X-ray AGN in Dynamically Active Massive Galaxy Clusters at z~1
  di: Muhibullah, Mustafa, et al.
  Pubblicazione: (2025)
• The Luminosity Function and Clustering of H$α$ Emitting Galaxies at $z\approx4-6$ from a Complete NIRCam Grism Redshift Survey
  di: Lin, Xiaojing, et al.
  Pubblicazione: (2025)
• The Quiescent Merging Nature of the Coma Cluster Revealed by ICM Velocity Structure
  di: Gatuzz, E., et al.
  Pubblicazione: (2025)
• XRISM Reveals Complex Multi-Temperature Structures in the Abell 2029 Galaxy Cluster
  di: Sarkar, Arnab, et al.
  Pubblicazione: (2025)