Showing 1–20 of 29 results
/ Date/ Name
Dec 20, 1998Making Damped Lyman Alpha Systems in Semi-Analytic ModelsAug 28, 2017Spatial Clustering of Dark Matter Halos: Secondary Bias, Neighbor Bias, and the Influence of Massive Neighbors on Halo PropertiesMay 10, 2001Modeling Angular-Momentum History in Dark-Matter HalosJan 14, 2013Angular Momentum Acquisition in Galaxy HalosJan 29, 2008Intrinsic Properties of Low-z SDSS GalaxiesJan 29, 2008Halo Mergers, Galaxy Mergers, and Why Hubble Type Depends on MassDec 10, 2008Redistributing hot gas around galaxies: do cool clouds signal a solution to the overcooling problem?Jan 28, 2009Gas-Rich Mergers in LCDM: Disk Survivability and the Baryonic Assembly of GalaxiesSep 5, 2018IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central GalaxiesOct 2, 2020IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and ObservationsJun 17, 2021IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of DustNov 11, 2002Damped Lyman alpha systems and galaxy formation models - II. High ions and Lyman limit systemsMar 26, 2003The Clustering Dipole of the Local Universe from the Two Micron All Sky SurveyNov 30, 2007Merger Histories of Galaxy Halos and Implications for Disk SurvivalFeb 24, 2000Optical Counterparts to Damped Lyman Alpha SystemsDec 9, 2010Observing the End of Cold Flow Accretion using Halo Absorption SystemsDec 5, 2018The Secondary Spin Bias of Dark Matter HaloesMay 29, 2013How to Zoom: Bias, Contamination, and Lagrange Volumes in Multimass Cosmological SimulationsFeb 24, 2000What Damped Ly-alpha Systems Tell Us About the Radial Distribution of Cold Gas at High RedshiftFeb 24, 2000Damped Ly-alpha Systems in Semi-Analytic Models: Sensitivity to dynamics, disk properties, and cosmology