Showing 1–20 of 20 results
/ Date/ Name
Oct 16, 2025The multimessenger view of Pulsar Timing Array black holes with the Horizon-AGN simulationSep 23, 2025Two-moment cosmic ray transport in RAMSESAug 25, 2025How Dust Models Shape High-z Galaxy Morphology: Insights from the NewCluster SimulationMay 16, 2025Redshift Evolution of the Intrinsic Alignments of Early-Type Galaxies and Subhalos in the Horizon Run 5 SimulationMar 17, 2025The Role of Large-Scale Environment in Shaping the Stellar Mass-Gas Metallicity Relation Across TimeDec 19, 2024Supermassive black hole growth in hierarchically merging nuclear star clustersDec 3, 2024Wandering and escaping: recoiling massive black holes in cosmological simulationsMay 16, 2024Formation pathways of the compact stellar systemsFeb 28, 2024Galaxies with grains: unraveling dust evolution and extinction curves with hydrodynamical simulationsMar 31, 2023LyAl-Net: A high-efficiency Lyman-$α$ forest simulation with a neural networkNov 2, 2022Translators of galaxy morphology indicators between observation and simulationSep 3, 2022How the super-Eddington regime affects black hole spin evolution in high-redshift galaxiesApr 26, 2022AGN jets do not prevent the suppression of conduction by the heat buoyancy instability in simulated galaxy clustersApr 7, 2022Cosmic rays and thermal instability in self-regulating cooling flows of massive galaxy clustersJan 21, 2022How the super-Eddington regime regulates black hole growth in high-redshift galaxiesJan 5, 2021Predicting the Observability of Population III Stars with ELT-HARMONI via the Helium $1640{\rmÅ}$ emission lineSep 22, 2020Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic timeJan 6, 2014Black hole evolution: II. Spinning black holes in a supernova-driven turbulent interstellar mediumDec 12, 2011Feeding compact bulges and supermassive black holes with low angular-momentum cosmic gas at high redshiftApr 1, 2011How AGN feedback and metal cooling shape cluster entropy profiles