Search Results - "Schaye, Joop"

The origin of scatter in the star formation rate–stellar mass relation by Matthee, Jorryt, Schaye, Joop

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Predictions for the relation between strong Hi absorbers and galaxies at redshift 3 by Rahmati, Alireza, Schaye, Joop

“…We combine cosmological, hydrodynamical simulations with accurate radiative transfer corrections to investigate the relation between strong absorbers ( ) and…”
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Star Formation Thresholds and Galaxy Edges: Why and Where by Schaye, Joop

“…We study global star formation thresholds in the outer parts of galaxies by investigating the stability of disk galaxies embedded in dark halos. The disks are…”
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Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra by van Daalen, Marcel P, McCarthy, Ian G, Schaye, Joop

“…ABSTRACT Upcoming weak lensing surveys require a detailed theoretical understanding of the matter power spectrum in order to derive accurate and precise…”
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Resolved galaxy scaling relations in the eagle simulation: star formation, metallicity, and stellar mass on kpc scales by Trayford, James W, Schaye, Joop

“…Abstract We explore scaling relations between the physical properties of spatially resolved regions within the galaxies that emerge in the Evolution and…”
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Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes by Ludlow, Aaron D, Schaye, Joop, Bower, Richard

“…ABSTRACT We study the impact of numerical parameters on the properties of cold dark matter haloes formed in collisionless cosmological simulations. We quantify…”
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Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests by Booth, C. M., Schaye, Joop

“…We present a method that self-consistently tracks the growth of supermassive black holes (BHs) and the feedback from active galactic nuclei (AGN) in…”
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The bahamas project: calibrated hydrodynamical simulations for large-scale structure cosmology by McCarthy, Ian G, Schaye, Joop, Bird, Simeon, Le Brun, Amandine MC

“…The evolution of the large-scale distribution of matter is sensitive to a variety of fundamental parameters that characterize the dark matter, dark energy, and…”
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Non-equilibirum ionization and cooling of metal-enriched gas in the presence of a photoionization background by Oppenheimer, Benjamin D., Schaye, Joop

“…Simulations of the formation of galaxies, as well as ionization models used to interpret observations of quasar absorption lines, generally either assume…”
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The separate and combined effects of baryon physics and neutrino free streaming on large-scale structure by Mummery, Benjamin O., McCarthy, Ian G., Bird, Simeon, Schaye, Joop

“…Abstract We use the cosmo-OWLS and bahamas suites of cosmological hydrodynamical simulations to explore the separate and combined effects of baryon physics…”
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The mean free path of hydrogen ionizing photons during the epoch of reionization by Rahmati, Alireza, Schaye, Joop

“…ABSTRACT We use the Aurora radiation-hydrodynamical simulations to study the mean free path (MFP) for hydrogen ionizing photons during the epoch of…”
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On the relation between the Schmidt and Kennicutt–Schmidt star formation laws and its implications for numerical simulations by Schaye, Joop, Dalla Vecchia, Claudio

“…When averaged over large scales, star formation in galaxies is observed to follow the empirical Kennicutt–Schmidt (KS) law for surface densities above a…”
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The BAHAMAS project: the CMB–large-scale structure tension and the roles of massive neutrinos and galaxy formation by McCarthy, Ian G, Bird, Simeon, Schaye, Joop, Harnois-Deraps, Joachim, Font, Andreea S, van Waerbeke, Ludovic

“…Abstract Recent studies have presented evidence for tension between the constraints on Ωm and σ8 from the cosmic microwave background (CMB) and measurements of…”
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On the evolution of the H i column density distribution in cosmological simulations by Rahmati, Alireza, Pawlik, Andreas H., Rai evic̀, Milan, Schaye, Joop

“…We use a set of cosmological simulations combined with radiative transfer calculations to investigate the distribution of neutral hydrogen in the…”
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The effects of metallicity, UV radiation and non-equilibrium chemistry in high-resolution simulations of galaxies by Richings, A. J., Schaye, Joop

“…We present a series of hydrodynamic simulations of isolated galaxies with stellar mass of 109 M⊙. The models use a resolution of 750 M⊙ per particle and…”
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The impact of the observed baryon distribution in haloes on the total matter power spectrum by Debackere, Stijn N B, Schaye, Joop, Hoekstra, Henk

“…ABSTRACT The interpretation of upcoming weak gravitational lensing surveys depends critically on our understanding of the matter power spectrum on scales $k…”
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How baryons can significantly bias cluster count cosmology by Debackere, Stijn N B, Schaye, Joop, Hoekstra, Henk

“…ABSTRACT We quantify two main pathways through which baryonic physics biases cluster count cosmology. We create mock cluster samples that reproduce the baryon…”
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The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end by Bower, Richard G, Schaye, Joop, Frenk, Carlos S, Theuns, Tom, Schaller, Matthieu, Crain, Robert A, McAlpine, Stuart

“…Galaxies fall into two clearly distinct types: 'blue-sequence' galaxies which are rapidly forming young stars, and 'red-sequence' galaxies in which star…”
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The accretion history of dark matter haloes – III. A physical model for the concentration–mass relation by Correa, Camila A., Wyithe, J. Stuart B., Schaye, Joop, Duffy, Alan R.

“…We present a semi-analytic, physically motivated model for dark matter halo concentration as a function of halo mass and redshift. The semi-analytic model…”
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The origin of scatter in the stellar mass–halo mass relation of central galaxies in the EAGLE simulation by Matthee, Jorryt, Schaye, Joop, Crain, Robert A, Schaller, Matthieu, Bower, Richard, Theuns, Tom

“…We use the hydrodynamical EAGLE simulation to study the magnitude and origin of the scatter in the stellar mass-halo mass relation for central galaxies. We…”
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