Joop Schaye

Leiden University — Netherlands

Physics and Astronomy · Physical Sciences

107h-index46.3kcitations788works8.82yr avg
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Research Topics

Galaxies: Formation, Evolution, Phenomena(569), Astronomy and Astrophysical Research(341), Astrophysics and Star Formation Studies(217), Stellar, planetary, and galactic studies(170), Astrophysics and Cosmic Phenomena(111)

Publications766 total

Under Pressure: UV Emission Line Ratios as Barometers of AGN Feedback Mechanisms
ArXiv.org·2026Open Access
Under Pressure: UV Emission Line Ratios as Barometers of AGN Feedback Mechanisms
arXiv (Cornell University)·2026Open Access
Gravitational potential drives the concentration dependence of the stellar mass–halo mass relation
Monthly Notices of the Royal Astronomical Society·2026Open Access
Gravitational potential drives the concentration dependence of the stellar mass–halo mass relation
Monthly Notices of the Royal Astronomical Society·2026Open Access
Luminosity-dependent assembly bias of brightest cluster galaxies from weak lensing and clustering
Physical review. D/Physical review. D.·2026· 1 citedOpen Access
Unveiling the properties and origin of massive quenched galaxies at $z\ge2$ in the COLIBRE hydrodynamical simulations
arXiv (Cornell University)·2025Open Access
The suppression of the matter power spectrum: strong feedback from X-ray gas mass fractions, kSZ effect profiles, and galaxy-galaxy lensing
arXiv (Cornell University)·2025Open Access
Ripples in the baryon to dark matter ratio in $Λ$CDM: implications for galaxy formation
arXiv (Cornell University)·2025Open Access
The impact of galaxy bias on cross-correlation tomography
Monthly Notices of the Royal Astronomical Society·2025Open Access
The resummation model in FLAMINGO: precisely predicting matter power suppression from observed halo baryon fractions
Monthly Notices of the Royal Astronomical Society·2025Open Access
MUSEQuBES: the column density, covering fraction, mass, and environmental dependence of cool H  <scp>i</scp> gas around low-redshift galaxies
Monthly Notices of the Royal Astronomical Society·2025Open Access
Signatures of dynamical activity in the hot gas profiles of groups and clusters in the FLAMINGO simulations
Monthly Notices of the Royal Astronomical Society·2025· 1 citedOpen Access
Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
Monthly Notices of the Royal Astronomical Society·2025Open Access
Euclid Quick Data Release (Q1): Identification of massive galaxy candidates at the end of the Epoch of Reionisation
ArXiv.org·2025Open Access
Think inside the box: cosmic variance and large-scale conformity of high-redshift massive galaxies in the FLAMINGO simulations
arXiv (Cornell University)·2025Open Access
The origin of scatter in the X-ray luminosity - halo mass relation of galaxy clusters
arXiv (Cornell University)·2025Open Access
A 1-per cent-accurate method to include baryonic effects in galaxy–galaxy lensing models
Monthly Notices of the Royal Astronomical Society·2025· 2 citedOpen Access
Euclid Quick Data Release (Q1). Quenching precedes bulge formation in dense environments but follows it in the field
ArXiv.org·2025Open Access
<i>Euclid</i> : An emulator for baryonic effects on the matter bispectrum
Astronomy and Astrophysics·2025Open Access
Baryonification II: constraining feedback with X-ray and kinematic Sunyaev-Zel'dovich observations
Journal of Cosmology and Astroparticle Physics·2025· 3 cited
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Frequent Co-authors

Tom Theuns(25), Robert A. Crain(23), R. G. Bower(20), Matthieu Schaller(20), Claudio Dalla Vecchia(20), Carlos S. Frenk(17), Ian G. McCarthy(16), Michelle Furlong(14), Adrian Jenkins(12), James W. Trayford(10), Simon D. M. White(8), John Helly(7), Julio F. Navarro(7), Yetli Rosas-Guevara(5), C. M. Booth(5), Till Sawala(5), Yan Qu(4), Roland Bacon(4), J. Brinchmann(4), T. Contini(4)