Inferring Halo Mass and Scale Radius of Galaxy Clusters Using Convolutional Neural Networks and Uchuu-UniverseMachine Catalogs

Documenti analoghi

• Quantifying the Velocity Anisotropy Profile of Galaxy Clusters Using the Uchuu Cosmological Simulation
  di: Abdullah, Mohamed H., et al.
  Pubblicazione: (2025)
• MPI-Rockstar: a Hybrid MPI and OpenMP Parallel Implementation of the Rockstar Halo finder
  di: Tokuue, Tomoyuki, et al.
  Pubblicazione: (2024)
• Optimizing the Gravitational Tree Algorithm for Many-Core Processors
  di: Tokuue, Tomoyuki, et al.
  Pubblicazione: (2023)
• Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks
  di: Garuda, Nikhil, et al.
  Pubblicazione: (2024)
• Constraining Cosmological Parameters using the Cluster Mass-Richness Relation
  di: Abdullah, Mohamed H., et al.
  Pubblicazione: (2022)