LH
Lars Hernquist
astro-ph.GAastro-ph.COastro-phastro-ph.HEastro-ph.IMhep-phastro-ph.SRcs.LGastro-ph.EPhep-th
On Valency
published · living versionsW_8v2wnrnw·v1 · currentpublished
Fast, Slow, Early, Late: Quenching Massive Galaxies at z~0.8
with Sandro Tacchella, Charlie Conroy, S. M. Faber, Benjamin D. Johnson +12
1 version
Preprints & journals
635 papers in the corpus · 1994–2026Mergers may not be the main channel for galaxy stellar mass growth at redshift : Predictions from cosmological hierarchical models and simulations2610.17575v1 · Hao Fu, Mohammadreza Ayromlou, Francesco Shankar et al.2026 · 0 citationsarXiv
The assembly history of NGC 1365 through chemical archaeology2609.40160v1 · Lisa J. Kewley, Kathryn Grasha, Alex Garcia et al.2026 · 1 citationNature Astronomy 2026, Volume 10, p. 892-900
JADES: Dynamical Measurements of Dark Matter Halo Masses at Using Galaxy Pairs2609.17756v1 · Zihao Wu, Daniel J. Eisenstein, Benjamin D. Johnson et al.2026 · 0 citationsarXiv
Common Excitation Patterns of Star Formation, Active Galactic Nuclei, and Shocks in Seyfert Galaxies2609.15913v1 · Peixin Zhu, Lisa J. Kewley, Dominika Ł. Kr'ol et al.2026 · 0 citationsarXiv
The Mass Dependence of the Fundamental Metallicity Relation in Observations and Simulations2608.24826v1 · Laura Carnevale, Alex M. Garcia, Paul Torrey et al.2026 · 0 citationsarXiv
The THESAN-ZOOM project: clumpiness of high-redshift galaxies and its connection to bursty star formation2608.19308v1 · Zihao Wang, Xuejian Shen, Rahul Kannan et al.2026 · 0 citationsarXiv
The Thesan-Zoom project: bursty star formation is incompatible with prolonged dust survival2607.08824v1 · Enrico Garaldi, Filip Popovic, Rahul Kannan et al.2026 · 0 citationsarXiv
Strong Stellar Diffusion from Wave DM Cosmological Simulation and Potential Unified Origin for dSphs, UFGs, and UDGs2606.30078v1 · A. Pozo, T. Broadhurst, J. Zhang et al.2026 · 0 citationsarXiv
TNG SAM: Bridging Hydrodynamical Complexity and Semi-Analytic Efficiency to Model Galaxy Formation2606.18352v1 · Osase Omoruyi, Bryan A. Terrazas, Yossi Oren et al.2026 · 0 citationsarXiv
The Lumina Project: Intergalactic Clumping and Recombination Sinks2606.18382v2 · Ali Sadain, Aaron Smith, Oliver Zier et al.2026 · 0 citationsarXiv
Supermassive Black Hole Assembly from Heavy Seeds with Dynamical Friction in the BRAHMA Simulations: Implications for JWST, LISA, and the Local Universe2606.12851v1 · Aklant K. Bhowmick, Laura Blecha, Paul Torrey et al.2026 · 0 citationsarXiv
Learning the Universe with PRFM-vol: Introducing a new subgrid model for star formation in cosmological simulations2606.10022v2 · Jan D. Burger, Volker Springel, Eve C. Ostriker et al.2026 · 0 citationsMonthly Notices of the Royal Astronomical Society, Volume 552, Issue 3, November 2026, stag1778
Learning the Universe at High Redshifts: Impact of Accretion Modeling on Early Black Hole Growth2606.10036v2 · Jonathan Kho, Aklant K. Bhowmick, Rainer Weinberger et al.2026 · 0 citationsarXiv
The Lumina Project: The Demographics of Active Galactic Nuclei from Quasars to Little Red Dots at 2605.24112v1 · Xuejian Shen, Oliver Zier, Aaron Smith et al.2026 · 1 citationarXiv
Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization2605.15310v2 · Oliver Zier, Aaron Smith, Xuejian Shen et al.2026 · 0 citationsarXiv
Unmasking Stellar Feedback-Driven Bubbles: Identification and Properties Analysis2605.08534v1 · Aaron Angress, Michael M. Foley, Sarah M. R. Jeffreson et al.2026 · 0 citationsarXiv
The evolution of the baryonic content and mass profiles of satellite galaxies in the MTNG simulations2604.24837v1 · Sergio Contreras, Raul E. Angulo, Giovanni Arico et al.2026 · 0 citationsarXiv
Cosmological constraints from the small scale clustering of Emission Line Galaxies2604.19449v2 · Sara Ortega-Martinez, Raul E. Angulo, Sergio Contreras et al.2026 · 0 citationsarXiv
Unraveling Chemical Enrichment in Extreme Emission-Line Galaxies: A Multi-Element Bayesian View of Bursty Star Formation and Galaxy Evolution in DESI2604.20060v1 · Razieh Emami, James A. A. Trussler, Tiger Yu-Yang Hsiao et al.2026 · 0 citationsarXiv
Introducing sapphire: Towards Hybrid Physics-Informed, Data-Driven Modeling of Galaxy Formation2604.06318v2 · Viraj Pandya, Greg L. Bryan, T. Lucas Makinen et al.2026 · 0 citationsarXiv
First results of AMBRA: Abundant Seeds and Early Mergers as a Pathway to the First Massive Black Holes2604.01123v2 · Yihao Zhou, Aklant Kumar Bhowmick, Tiziana Di Matteo et al.2026 · 0 citationsarXiv
The birth of the intracluster medium: the evolution of multiphase gas and Lyman- haloes in a simulated protocluster2603.16991v2 · Jake S. Bennett, Aaron Smith, Fabrizio Arrigoni-Battaia et al.2026 · 0 citationsarXiv
ENhanced Galactic Atmospheres With Arepo: Resolving the CGM at 200 pc with the ENGAWA Simulations2603.05584v2 · Scott Lucchini, Cecilia Abramson, Cameron Hummels et al.2026 · 0 citationsarXiv
Correlated residuals in Tully-Fisher and Fundamental Plane relations and their impact on peculiar velocity measurements2602.23033v1 · Tyann Dumerchat, Raul E. Angulo, Julian Bautista et al.2026 · 0 citationsarXiv
Implications of the nanoHertz Gravitational-Wave Background for Galactic Feedback and Massive Black Hole Growth2602.15938v2 · Megan Taylor Tillman, Blakesley Burkhart, Chiara M. F. Mingarelli et al.2026 · 0 citationsarXiv
What Suppresses Star Formation in Bulge-Dominated Early-Type Galaxies?2602.12324v1 · Lori E. Porter, S. M. R. Jeffreson, Greg L. Bryan et al.2026 · 0 citationsarXiv
ICM-SHOX III. The case of MACS J0018.5+1626, a radio relic that looks like a radio halo?2602.05050v2 · P. Dom'inguez-Fern'andez, J. A. ZuHone, E. M. Silich et al.2026 · 0 citationsarXiv
The effect of baryons on the positions and velocities of satellite galaxies in the MTNG simulation2512.04080v1 · Sergio Contreras, Raul E. Angulo, Sownak Bose et al.2025 · 2 citationsarXiv
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties Are Smaller Than They Appear.41349072 · Folsom, Dylan, Blanco, Carlos, Lisanti, Mariangela et al.2025 · 5 citationsPhysical review letters. 2025;135(21):211004
AGN feedback in merging galaxies with a SMUGGLE multiphase ISM2511.13024v1 · Aneesh Sivasankaran, Laura Blecha, Paul Torrey et al.2025 · 0 citationsarXiv
Synthetic JWST galaxy images in the TNG50 simulation - I. Model validation and comparison to observations2511.04780v1 · Alejandro Guzm'an-Ortega, Gustavo Bruzual, Vicente Rodriguez-Gomez et al.2025 · 2 citationsarXiv
Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift2510.26877v2 · Alex M. Garcia, Paul Torrey, Aniket Bhagwat et al.2025 · 6 citationsarXiv
Modeling gravitational wave sources in the MillenniumTNG simulations2510.06311v2 · Federico Marinacci, Marco Baldi, Giuliano Iorio et al.2025 · 1 citationarXiv
Heavy seeds and the first black holes: Insights from the BRAHMA simulations2510.01322v1 · Aklant K. Bhowmick, Laura Blecha, Paul Torrey et al.2025 · 7 citationsarXiv
The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics2509.19427v1 · Xuejian Shen, Oliver Zier, Mark Vogelsberger et al.2025 · 1 citationMon Not R Astron Soc (2026)
Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters2509.07078v2 · Mark R. Lovell, Annalisa Pillepich, Christoph Engler et al.2025 · 3 citationsMon Not R Astron Soc (2025) 4367-4389
Little Red Dots Are Nurseries of Massive Black Holes2509.02664v2 · Fabio Pacucci, Lars Hernquist, Michiko Fujii2025 · 19 citationsThe Astrophysical Journal, 2025, Volume 994, Number 40
How does feedback affect the star formation histories of galaxies?2508.21152v1 · Kartheik G. Iyer, Tjitske K. Starkenburg, Greg L. Bryan et al.2025 · 7 citationsarXiv
Development of Turbulence in Post-shock Regions2508.13291v1 · Michael M. Foley, Philip Mocz, Blakesley Burkhart et al.2025 · 1 citationarXiv
Measuring the splashback feature: Dependence on halo properties and history2507.22102v2 · Qiaorong S. Yu, Stephanie O'Neil, Xuejian Shen et al.2025 · 1 citationThe Open Journal of Astrophysics, 8 (2025)
Invisible Accretion: Ionized Envelopes of TNG50 HVCs can Sustain Star Formation2507.18687v1 · Scott Lucchini, Jiwon Jesse Han, Lars Hernquist et al.2025 · 4 citationsarXiv
The THESAN project: environmental drivers of Local Group reionization2507.16245v1 · Yu Zhao, Aaron Smith, Rahul Kannan et al.2025 · 2 citationsarXiv
Ray-tracing Fast Radio Bursts Through IllustrisTNG: Cosmological Dispersion Measures from Redshift 0 to 5.52507.07090v2 · Ralf M. Konietzka, Liam Connor, Vadim A. Semenov et al.2025 · 0 citationsarXiv
Photometric analysis of the intracluster light in the TNG300 simulation and wide-field observations2507.02105v1 · Daniel Montenegro-Taborda, Vicente Rodriguez-Gomez, Vladimir Avila-Reese et al.2025 · 3 citationsarXiv
Infalling ultra-faint dwarfs as emissaries of the Axiverse2506.16915v2 · A. Pozo, T. Broadhurst, H. N. Luu et al.2025 · 0 citationsA&A 704, A34 (2025)
Dynamics of low-mass black hole seeds in the BRAHMA simulations using subgrid-dynamical friction: Impact on merger-driven black hole growth in the high redshift Universe2506.09184v1 · Aklant K. Bhowmick, Laura Blecha, Luke Z. Kelley et al.2025 · 8 citationsarXiv
Fully non-linear simulations of galaxy intrinsic alignments for weak lensing with the MillenniumTNG lightcone2505.15882v1 · Fulvio Ferlito, Volker Springel, Christopher T. Davies et al.2025 · 3 citationsarXiv
The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts2505.05554v1 · Zihao Wang, Xuejian Shen, Mark Vogelsberger et al.2025 · 12 citationsMon Not R Astron Soc (2025) 2675-2697
High-redshift Millennium and Astrid galaxies in effective field theory at the field level2505.03626v1 · James M. Sullivan, Carolina Cuesta-Lazaro, Mikhail M. Ivanov et al.2025 · 8 citationsarXiv
MISTRAL: a model for AGN winds from radiatively efficient accretion in cosmological simulations2504.08041v2 · Marion Farcy, Michaela Hirschmann, Rachel S. Somerville et al.2025 · 11 citationsMon Not R Astron Soc (2025) 967-993
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