Robert Feldmann

University of Zurich — Switzerland

Physics and Astronomy · Physical Sciences

59h-index12.5kcitations264works18.12yr avg
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Research Topics

Galaxies: Formation, Evolution, Phenomena(154), Astronomy and Astrophysical Research(122), Stellar, planetary, and galactic studies(62), Astrophysics and Star Formation Studies(54), Gamma-ray bursts and supernovae(30)

Publications264 total

SQuIGG <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mover> <mml:mrow> <mml:mi>L</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>→</mml:mo> </mml:mrow> </mml:mover> </mml:math> E: Buried Star Formation Cannot Explain the Rapidly Fading CO(2–1) Luminosity in Massive, <i>z</i> ∼ 0.7 Post-starburst Galaxies
The Astronomical Journal·2025Open Access
Towards Reconciling Reionization with JWST: The Role of Bright Galaxies and Strong Feedback
ArXiv.org·2025Open Access
The AGORA High-resolution Galaxy Simulations Comparison Project. X: Formation and Evolution of Galaxies at the High-redshift Frontier
arXiv (Cornell University)·2025Open Access
Igniting galaxy formation in the post-reionization universe
arXiv (Cornell University)·2025Open Access
Unusually High Gas-to-dust Ratios Observed in High-redshift Quiescent Galaxies
The Astrophysical Journal Letters·2025· 1 citedOpen Access
The Structure and Formation Histories of Low-mass Quiescent Galaxies in the A2744 Cluster Environment
The Astrophysical Journal·2025· 2 citedOpen Access
Discs no more: the morphology of low-mass simulated galaxies in FIREbox
Monthly Notices of the Royal Astronomical Society·2025· 1 citedOpen Access
Rise of the forsaken relics: connecting present-day stellar streams and phase-mixed galaxies to the Epoch of Reionization
arXiv (Cornell University)·2025Open Access
Discovery of red galaxy candidates at z ~ 12: Early dust growth or significant nebular emission with high-temperature stars?
arXiv (Cornell University)·2025Open Access
Explaining the Weak Evolution of the High-redshift Mass–Metallicity Relation with Galaxy Burst Cycles
The Astrophysical Journal Letters·2025Open Access
Quenching through Tidal Gas Removal: Molecular Gas and Star Formation in Tidal Tails of <i>z</i> ∼ 0.7 Post-starburst Galaxies
The Astrophysical Journal·2025· 2 citedOpen Access
UNCOVER/MegaScience: No Evidence of Environmental Quenching in a <i>z </i>∼ 2.6 Protocluster
The Astrophysical Journal Letters·2025· 3 citedOpen Access
SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies
arXiv (Cornell University)·2025Open Access
Great Balls of FIRE
Astronomy and Astrophysics·2025· 3 citedOpen Access
Disks no more: the morphology of low-mass simulated galaxies in FIREbox
arXiv (Cornell University)·2025Open Access
JWST UNCOVERs the Optical Size–Stellar Mass Relation at 4 &lt; <i>z</i> &lt; 8: Rapid Growth in the Sizes of Low-mass Galaxies in the First Billion Years of the Universe
The Astrophysical Journal·2025· 10 citedOpen Access
Unusually High Gas-to-Dust Ratios Observed in High-Redshift Quiescent Galaxies
arXiv (Cornell University)·2025Open Access
Cosmological Simulations of Galaxies
arXiv (Cornell University)·2025Open Access
Unveiling the dark Universe with HI and EMBER-2
arXiv (Cornell University)·2025Open Access
Cosmological simulations of galaxies
Elsevier eBooks·2025· 1 cited
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Frequent Co-authors

Philip F. Hopkins(23), Dušan Kereš(23), Claude‐André Faucher‐Giguère(23), Eliot Quataert(17), Christopher C. Hayward(13), Andrew Wetzel(10), Xiangcheng Ma(10), Daniel Anglés‐Alcázar(9), Rachel Bezanson(9), A. Renzini(8), Jenny E. Greene(8), Ivo Labbé(8), Lukas J. Furtak(8), Bingjie Wang(8), Hakim Atek(8), Gabriel Brammer(8), Seiji Fujimoto(8), Joel Leja(8), Pascal A. Oesch(8), Richard Pan(8)