about
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The Athena X-ray Integral Field Unit (X-IFU)On the galaxy–halo connection in the EAGLE simulationImpact of baryon physics on dark matter structures: a detailed simulation study of halo density profilesObservations of the missing baryons in the warm–hot intergalactic mediumInitial deep LOFAR observations of epoch of reionization windowsThe Lyα Forest Power Spectrum from the Sloan Digital Sky SurveyThermal history and metal enrichment of the intergalactic mediumUpper Limits on the 21 cm Epoch of Reionization Power Spectrum from One Night with LOFARSimulating the 21 cm forest detectable with LOFAR and SKA in the spectra of high-zGRBsPolarization leakage in epoch of reionization windows – I. Low Frequency Array observations of the 3C196 fieldConstraining the epoch of reionization with the variance statistic: simulations of the LOFAR caseProbing reionization with LOFAR using 21-cm redshift space distortionsGlobal structure and kinematics of stellar haloes in cosmological hydrodynamic simulationsDark matter halo concentrations in theWilkinson Microwave Anisotropy Probeyear 5 cosmologyErratum: Dark matter halo concentrations in the Wilkinson Microwave Anisotropy Probe year 5 cosmologyThe physics driving the cosmic star formation historyModelling neutral hydrogen in galaxies using cosmological hydrodynamical simulationsThe impact of baryons on the spins and shapes of dark matter haloesThe accretion history of dark matter haloes – I. The physical origin of the universal functionThe accretion history of dark matter haloes – II. The connections with the mass power spectrum and the density profileThe accretion history of dark matter haloes – III. A physical model for the concentration–mass relationOptical colours and spectral indices of z = 0.1 eagle galaxies with the 3D dust radiative transfer code skirtBarred galaxies in the EAGLE cosmological hydrodynamical simulationProperties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologiesWinds of change: reionization by starburst galaxiesMass-Discrepancy Acceleration Relation: A Natural Outcome of Galaxy Formation in Cold Dark Matter HalosThe properties of ‘dark’ ΛCDM haloes in the Local GroupSize matters: abundance matching, galaxy sizes, and the Tully–Fisher relation in EAGLEThe dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an endThe oldest and most metal-poor stars in the APOSTLE Local Group simulationsA chronicle of galaxy mass assembly in the EAGLE simulationThe low-mass end of the baryonic Tully–Fisher relationGalaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical modelsSupermassive black holes in the EAGLE Universe. Revealing the observables of their growthThe effect of baryons on redshift space distortions and cosmic density and velocity fields in the EAGLE simulationAlignments between galaxies, satellite systems and haloesThe link between the assembly of the inner dark matter halo and the angular momentum evolution of galaxies in the EAGLE simulationPredictions of hydrodynamic simulations for direct dark matter detectionSimulated Milky Way analogues: implications for dark matter direct searchesThe Fermi GeV excess: challenges for the dark matter interpretation
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P50
description
Nederlands astronoom en hoogleraar
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americký astronom
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hulumtues
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ricercatore
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հետազոտող
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Joop Schaye
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Joop Schaye
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Joop Schaye
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P106
P1006
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P1412
P1559
Joop Schaye
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P19
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0000-0002-0668-5560
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1973-06-29T00:00:00Z
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