Publication data of Hahn, Oliver: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2006200820102012201420162018202020222024010002000300040005000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications200620082010201220142016201820202022202402040608010002.557.51012.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion2006200820102012201420162018202020222024010203040
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestA new approach to simulating collisionless dark matter fluidsAccurate initial conditions for cosmological N-body simulations: Minimizing truncation and discreteness errorsAccurate initial conditions for cosmological N-body simulations: Minimizing tr…Four phases of angular-momentum buildup in high-z galaxies: from cosmic-web streams through an extended ring to disc and bulgeFour phases of angular-momentum buildup in high-z galaxies: from cosmic-w…Mergers and Mass Accretion for Infalling Halos Both End Well Outside Cluster Virial RadiiMergers and Mass Accretion for Infalling Halos Both End Well Outside Cluster …How to Zoom: Bias, Contamination, and Lagrange Volumes in Multimass Cosmological SimulationsHow to Zoom: Bias, Contamination, and Lagrange Volumes in Multimass Cos…Halo assembly bias and the tidal anisotropy of the local halo environmentThe Properties of Cosmic Velocity FieldsThe Large-Scale Orientations of Disk GalaxiesHalo-to-Halo Similarity and Scatter in the Velocity Distribution of Dark MatterThe Tidal Origin of the Environment Dependence of Halo AssemblyLarge-scale dark matter simulationsThe Warm DM halo mass function below the cut-off scaleTracing the Dark Matter Sheet in Phase SpaceThe Aspen--Amsterdam Void Finder Comparison ProjectUniversal halo mass function and scale-dependent bias from N-body simulations with non-Gaussian initial conditionsUniversal halo mass function and scale-dependent bias from N-body simulati…The Evolution of Dark Matter Halo Properties in Clusters, Filaments, Sheets and VoidsThe Evolution of Dark Matter Halo Properties in Clusters, Filaments, Sheets an…Disruption of Dark Matter Substructure: Fact or Fiction?Properties of Dark Matter Haloes in Clusters, Filaments, Sheets and VoidsMulti-scale initial conditions for cosmological simulations2006200820102012201420162018202020222024010002000300040005000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)A new approach to simulating collisionless dark matter fluidsAccurate initial conditions for cosmological N-body simulations: Minimizing truncation and discreteness errorsAccurate initial conditions for cosmological N-body simulations: Minimizing tr…Four phases of angular-momentum buildup in high-z galaxies: from cosmic-web streams through an extended ring to disc and bulgeFour phases of angular-momentum buildup in high-z galaxies: from cosmic-w…Mergers and Mass Accretion for Infalling Halos Both End Well Outside Cluster Virial RadiiMergers and Mass Accretion for Infalling Halos Both End Well Outside Cluster …How to Zoom: Bias, Contamination, and Lagrange Volumes in Multimass Cosmological SimulationsHow to Zoom: Bias, Contamination, and Lagrange Volumes in Multimass Cos…Halo assembly bias and the tidal anisotropy of the local halo environmentThe Properties of Cosmic Velocity FieldsThe Large-Scale Orientations of Disk GalaxiesHalo-to-Halo Similarity and Scatter in the Velocity Distribution of Dark MatterThe Tidal Origin of the Environment Dependence of Halo AssemblyLarge-scale dark matter simulationsThe Warm DM halo mass function below the cut-off scaleTracing the Dark Matter Sheet in Phase SpaceThe Aspen--Amsterdam Void Finder Comparison ProjectUniversal halo mass function and scale-dependent bias from N-body simulations with non-Gaussian initial conditionsUniversal halo mass function and scale-dependent bias from N-body simulati…The Evolution of Dark Matter Halo Properties in Clusters, Filaments, Sheets and VoidsThe Evolution of Dark Matter Halo Properties in Clusters, Filaments, Sheets an…Disruption of Dark Matter Substructure: Fact or Fiction?Properties of Dark Matter Haloes in Clusters, Filaments, Sheets and VoidsMulti-scale initial conditions for cosmological simulations20062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average20062008201020122014201620182020202220240200400600800