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Rhapsody-G simulations I: the cool cores, hot gas and stellar content of massive galaxy clustersRhapsody-G simulations – II. Baryonic growth and metal enrichment in massive galaxy clustersProperties of dark matter haloes in clusters, filaments, sheets and voidsVirial scaling of galaxies in clusters: bright to faint is cool to hotThe buildup of the Hubble sequence in the cosmos fieldThe AGORA high-resolution galaxy simulations comparison projectRhapsody-G simulations: galaxy clusters as baryonic closed boxes and the covariance between hot gas and galaxiesMergers and mass accretion for infalling halos both end well outside cluster virial radiiRhapsody. II. Subhalo properties and the impact of tidal stripping from a statistical sample of cluster-size halosHalo-to-halo similarity and scatter in the velocity distribution of dark matterRhapsody. I. Structural properties and formation history from a statistical sample of re-simulated cluster-size halosThe Aspen–Amsterdam void finder comparison projectHow to zoom: bias, contamination and Lagrange volumes in multimass cosmological simulationsENZO: an adaptive mesh refinement code for astrophysicsSubstructure and merger detection in resolved NIKA Sunyaev-Zel’dovich images of distant clustersThe dependence of galaxy clustering on tidal environment in the Sloan Digital Sky SurveyHalo assembly bias and the tidal anisotropy of the local halo environmentDisruption of dark matter substructure: fact or fiction?What sets the central structure of dark matter haloes?Tracing the cosmic webEarth-mass haloes and the emergence of NFW density profilesTwo is better than one: joint statistics of density and velocity in concentric spheres as a cosmological probeCollisionless Dynamics and the Cosmic WebGeneral relativistic screening in cosmological simulationsAn adaptively refined phase–space element method for cosmological simulations and collisionless dynamicsThe properties of cosmic velocity fieldsFour phases of angular-momentum buildup in high-z galaxies: from cosmic-web streams through an extended ring to disc and bulgeTRACING, ANALYZING AND VISUALIZING DARK MATTER IN PHASE SPACEThe locations of halo formation and the peaks formalismThe warm dark matter halo mass function below the cut-off scaleA new approach to simulating collisionless dark matter fluidsHow closely do baryons follow dark matter on large scales?Population III star formation in large cosmological volumes. I. Halo temporal and physical environmentTracing the dark matter sheet in phase spaceCoplanar streams, pancakes and angular-momentum exchange in high-z disc galaxiesMulti-scale initial conditions for cosmological simulationsThe large-scale orientations of disc galaxiesHalo mass function and scale-dependent bias from N-body simulations with non-Gaussian initial conditionsLagrangian statistics of dark halos in a {Lambda}CDM cosmologyThe anisotropic two-point correlation functions of the nonlinear traceless tidal field in the principal-axis frame
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description
researcher ORCID ID = 0000-0001-9440-1152
@en
wetenschapper
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name
O. Hahn
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Oliver Hahn
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Oliver Hahn
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O. Hahn
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Oliver Hahn
@en
Oliver Hahn
@es
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O. Hahn
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O. Hahn
@nl
Oliver Hahn
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Oliver Hahn
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0000-0001-9440-1152