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UniverseMachine
Arxiv:2010.00693V2 [Astro-Ph.GA] 31 Oct 2020 Total Mass of Dark Matter Around Galaxies
The Diversity and Variability of Star Formation Histories in Different Simulations
Evolution of Galactic Star Formation in Galaxy Clusters and Post-Starburst Galaxies
It Is Feasible to Directly Measure Black Hole Masses in the First Galaxies
UC Berkeley UC Berkeley Electronic Theses and Dissertations
Arxiv:2109.00003V1 [Astro-Ph.CO] 31 Aug 2021
Unifying Observations and Simulations to Measure Dark Matter Accretion & (2) Inclusivity-Driven Designs for General-Education Astronomy Courses
Exploring the High-Mass End of the Stellar Mass Function of Star
Galaxy—Halo Modeling of Large-Scale Structure
The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
Virtual 'Universe Machine' Sheds Light on Galaxy Evolution 10 August 2019, by Daniel Stolte
Elementary Particles, Dark Matter, and Dark Energy: Descriptions That
II. Physical Properties and Scaling Relations for Galaxies at Z = 4-10
Astro2020 Science White Paper Dark Matter Science in the Era of LSST
Learning Effective Physical Laws for Generating Cosmological Hydrodynamics with Lagrangian Deep Learning Preprint, Compiled October 8, 2020
Carnegie Mellon University MELLON COLLEGE of SCIENCE
Axi-Higgs Cosmology
Chun-Hao To's Personal Webpage
Top View
Identification De La Matière Noire À L'ère Du Grand
Mock Innsbruck
Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
Stellar and Weak Lensing Profiles of Massive Galaxies in The