Dušan Kereš

UC San Diego Health System — United States

Physics and Astronomy · Physical Sciences

86h-index22.4kcitations238works5.92yr avg
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Research Topics

Galaxies: Formation, Evolution, Phenomena(194), Astronomy and Astrophysical Research(113), Astrophysics and Star Formation Studies(97), Stellar, planetary, and galactic studies(70), Astrophysics and Cosmic Phenomena(30)

Publications238 total

Discs no more: the morphology of low-mass simulated galaxies in FIREbox
Monthly Notices of the Royal Astronomical Society·2025· 1 citedOpen Access
The role of galactic winds fueling central starbursts and quasars in the FIRE cosmological simulations
arXiv (Cornell University)·2025Open Access
Galaxy Metallicity Gradients in the Reionization Epoch from the FIRE-2 Simulations
arXiv (Cornell University)·2025Open Access
Galactic Center Gamma-Ray Emission in MHD Galaxy Formation Simulations with Full Cosmic Ray Spectra
arXiv (Cornell University)·2025Open Access
Disks no more: the morphology of low-mass simulated galaxies in FIREbox
arXiv (Cornell University)·2025Open Access
The Physical Origin of Positive Metallicity Radial Gradients in High-redshift Galaxies: Insights from the FIRE-2 Cosmological Hydrodynamic Simulations
The Astrophysical Journal·2025· 2 citedOpen Access
Constraining cosmic ray transport models using circumgalactic medium properties and observables
arXiv (Cornell University)·2025Open Access
Hooks, Lines, and Sinkers: How Active Galactic Nucleus Feedback and Cosmic-Ray Transport Shape the Far-infrared–Radio Correlation of Galaxies
The Astrophysical Journal·2025· 5 citedOpen Access
A dusty dawn: galactic dust buildup at <i>z</i> ≳ 5
Monthly Notices of the Royal Astronomical Society·2025· 8 citedOpen Access
The Effect of Galaxy Interactions on Starbursts in Milky Way-mass Galaxies in FIRE Simulations
The Astrophysical Journal·2025· 3 citedOpen Access
Observational Signatures of AGN Feedback in the Morphology and the Ionization States of Milky Way-like Galaxies
The Astrophysical Journal·2024· 3 citedOpen Access
Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
Monthly Notices of the Royal Astronomical Society·2024· 24 citedOpen Access
Any way the wind blows: quantifying superbubbles and their outflows in simulated galaxies across <i>z</i> ≈ 0-3
Monthly Notices of the Royal Astronomical Society·2024· 4 citedOpen Access
The Effect of Galaxy Interactions on Starbursts in Milky Way-Mass Galaxies in FIRE Simulations
arXiv (Cornell University)·2024Open Access
Hooks, Lines, and Sinkers: How AGN Feedback and Cosmic-Ray Transport shape the Far Infrared-Radio Correlation of Galaxies
arXiv (Cornell University)·2024Open Access
Angular momentum transfer in cosmological simulations of Milky Way-mass discs
Monthly Notices of the Royal Astronomical Society·2024· 3 citedOpen Access
Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
arXiv (Cornell University)·2024· 3 citedOpen Access
Unravelling jet quenching criteria across L* galaxies and massive cluster ellipticals
Monthly Notices of the Royal Astronomical Society·2024· 13 citedOpen Access
Any Way the Wind Blows: Quantifying Superbubbles and their Outflows in Simulated Galaxies across $z \approx 0-3$
arXiv (Cornell University)·2024· 1 citedOpen Access
Angular momentum transfer in cosmological simulations of Milky Way-mass discs
arXiv (Cornell University)·2024· 1 citedOpen Access
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Frequent Co-authors

Philip F. Hopkins(39), Claude‐André Faucher‐Giguère(31), Eliot Quataert(25), Andrew Wetzel(15), Lars Hernquist(13), Norman Murray(12), Michael Boylan-Kolchin(11), Shea Garrison-Kimmel(10), Christopher C. Hayward(9), T K Chan(9), James S. Bullock(8), Xiangcheng Ma(8), Thomas J. Cox(6), José Oñorbe(6), Daniel Anglés‐Alcázar(6), Alexander L. Muratov(6), Cameron Hummels(5), Robert Feldmann(5), Coral Wheeler(5), Kareem El-Badry(5)