The Evolution of Half-Mass Radii and Color Gradients for Young and Old Quiescent Galaxies at $0.5 < z < 3$ with JWST/PRIMER

Documenti analoghi

• 3D-DASH: The Evolution of Size, Shape, and Intrinsic Scatter in Populations of Young and Old Quiescent Galaxies at 0.5 < z < 3
  di: Clausen, Maike, et al.
  Pubblicazione: (2024)
• JWST PRIMER: strong evidence for the environmental quenching of low-mass galaxies out to $\mathbf{\textit{z} \simeq 2}$
  di: Hamadouche, M. L., et al.
  Pubblicazione: (2024)
• No evidence (yet) for increased star-formation efficiency at early times
  di: Donnan, C. T., et al.
  Pubblicazione: (2025)
• An optimal ALMA image of the Hubble Ultra Deep Field in the era of JWST: obscured star formation and the cosmic far-infrared background
  di: Hill, Ryley, et al.
  Pubblicazione: (2023)
• Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms
  di: Carnall, A. C., et al.
  Pubblicazione: (2017)