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19932026
most citedProfiles of dark haloes: evolution, scatter, and environment

2.3k citations · 46.3k across the 327 of their papers we have counts for

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Showing astro-ph.GAShow all

179 papers · 1 filter

astro-ph.GA2026

The MAGE Project: Size Evolution and Disk Formation in Massive Galaxies at Cosmic Dawn

Zhiyuan Yao, Avishai Dekel, Romain Teyssier +5

We investigate size evolution and disk formation with a new suite of eleven cosmological zoom-in simulations, Massive Assembly of Galaxies in the Early universe (MAGE), run with RA…

astro-ph.GA2026

The AGORA High-resolution Galaxy Simulations Comparison Project. IX - Part 2: Effects of a Major Galaxy Merger on the Stellar Morphology of a Milky Way-mass Galaxy Progenitor

Thinh Huu Nguyen, Kirk S. S. Barrow, Minyong Jung +23

Galaxy mergers, with their high sensitivity to initial conditions, provide a valuable setting for comparative studies of galaxy simulation codes. Following our first paper focusing…

astro-ph.GA2026

The AGORA High-resolution Galaxy Simulations Comparison Project. IX - Part 1: Effects of a Major Galaxy Merger on Star Formation of a Milky Way-mass Galaxy Progenitor

Thinh Huu Nguyen, Kirk S. S. Barrow, Minyong Jung +23

Given their highly nonlinear dynamics and sensitivity to initial conditions, galaxy mergers are a compelling area to conduct a simulation code comparison. We perform a comparative…

astro-ph.GA2025★ 1 cited

Not all cores are equal: Phase-space origins of dynamical friction, stalling and buoyancy

Shashank Dattathri, Frank C. van den Bosch, Uddipan Banik +4

Dynamical friction governs the orbital decay of massive perturbers within galaxies and dark matter halos, yet its standard Chandrasekhar formulation fails in systems with cores of…

astro-ph.GA2025★ 1 cited

From Feedback-Free Star Clusters to Little Red Dots via Compaction

Avishai Dekel, Dhruba Dutta Chowdhury, Sharon Lapiner +6

We address the origin of the Little Red Dots (LRDs) seen by JWST at cosmic morning () as compact stellar systems with over-massive black holes (BHs). We propose…

astro-ph.GA2025★ 2 cited

The Relationship at : Big Black Holes in Little Red Dots

Brenda L. Jones, Dale D. Kocevski, Fabio Pacucci +25

JWST has identified a large population of faint, broad-line active galactic nuclei (AGN) in the early universe that are powered by black holes (BHs) that often appear overmassive r…

astro-ph.GA2025★ 6 cited

Investigating the Growth of Little Red Dot Descendants at z<4 with the JWST

Jean-Baptiste Billand, David Elbaz, Fabrizio Gentile +16

One of JWST's most remarkable discoveries is a population of compact red galaxies known as Little Red Dots (LRDs). Their existence raises many questions about their nature, origin,…

astro-ph.GA2025

A 13-Billion-Year View of Galaxy Growth: Metallicity Gradient Evolution from the Local Universe to with JWST and Archival Surveys

Zihao Li, Zheng Cai, Xin Wang +25

The galaxy gas-phase metallicity gradients have been extensively studied over the past four decades, both in the local and high-redshift universe, as they trace the baryon cycle an…

astro-ph.GA2025

From FFB Starbursts at Cosmic Dawn to Quenching at Cosmic Morning: Hi-z Galaxy Bimodality

Avishai Dekel, Nir Mandelker, Zhaozhou Li +5

We propose a mass-dependent bimodality in the early evolution of galaxies. The massive track connects the super-bright galaxies at cosmic dawn () to the super-massive quiesc…

astro-ph.GA2025★ 10 cited

The AGORA High-Resolution Galaxy Simulations Comparison Project VII: Satellite quenching in zoom-in simulation of a Milky Way-mass halo

R. Rodríguez-Cardoso, S. Roca-Fàbrega, Minyong Jung +19

Context: Satellite galaxies experience multiple physical processes when interacting with their host halos, often leading to the quenching of star formation. In the Local Group (LG)…

astro-ph.GA2025★ 4 cited

The AGORA High-resolution Galaxy Simulations Comparison Project. VIII: Disk Formation and Evolution of Simulated Milky Way Mass Galaxy Progenitors at

Minyong Jung, Ji-hoon Kim, Thinh H. Nguyen +24

We investigate how differences in the stellar feedback produce disks with different morphologies in Milky Way-like progenitors over 1 , using eight state-of-the-art…

astro-ph.GA2025★ 7 cited

Insights on Metal Enrichment and Environmental Effect at with JWST ASPIRE/EIGER and Chemical Evolution Model

Zihao Li, Koki Kakiichi, Lise Christensen +15

We present the mass-metallicity relation (MZR) for a parent sample of 604 galaxies at with \OIII\ doublets detected, using the deep JWST/NIRCam wide field slitless sp…

astro-ph.GA2025★ 3 cited

The rise of the galactic empire: luminosity functions at and estimated with the MIDISNGDEEP ultra-deep JWST/NIRCam dataset

Pablo G. Pérez-González, Göran Östlin, Luca Costantin +39

We present a sample of six F200W and three F277W dropout sources identified as galaxy candidates using the deepest JWST/NIRCam data to date (5 depths mag at…

astro-ph.GA2025★ 1 cited

The Cosmic Evolution Early Release Science Survey (CEERS)

Steven L. Finkelstein, Micaela B. Bagley, Pablo Arrabal Haro +96

We present the Cosmic Evolution Early Release Science (CEERS) Survey, a 77.2 hour Director's Discretionary Early Release Science Program. CEERS demonstrates, tests, and validates e…

astro-ph.GA2025★ 6 cited

On the origin of compressive turbulence in protoclumps in high redshift disks

Omry Ginzburg, Avishai Dekel, Nir Mandelker +4

The giant, star forming clumps in gas-rich, high redshift disks are commonly assumed to form due to gravitational instabilities, in which protoclumps have a Toomre- parameter le…

astro-ph.GA2024

Effects of Cloud Geometry and Metallicity on Shattering and Coagulation of Cold Gas, and Implications for Cold Streams Penetrating Virial Shocks

Zhiyuan Yao, Nir Mandelker, S. Peng Oh +2

Theory and observations reveal that the circumgalactic medium (CGM) and the cosmic web at high redshifts are multiphase, with small clouds of cold gas embedded in a hot, diffuse me…

astro-ph.GA2024★ 9 cited

On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn

Zachary Lee Andalman, Romain Teyssier, Avishai Dekel

Motivated by the early excess of bright galaxies seen by JWST, we run zoom-in cosmological simulations of a massive galaxy at Cosmic Dawn, in a halo of at …

astro-ph.GA2024★ 18 cited

Growth of Massive Black-Holes in FFB Galaxies at Cosmic Dawn

Avishai Dekel, Nicholas C. Stone, Dhruba Dutta Chowdhury +4

The scenario of feedback-free starbursts (FFB), which predicts excessively bright galaxies at cosmic dawn as observed using JWST, may provide a natural setting for black hole (BH)…

astro-ph.GA2024★ 1 cited

Radial Transport in High-Redshift Disk Galaxies Dominated by Inflowing Streams

Dhruba Dutta Chowdhury, Avishai Dekel, Nir Mandelker +2

We study the radial transport of cold gas within simulated disk galaxies at cosmic noon, aiming at distinguishing between disk instability and accretion along cold streams from the…

astro-ph.GA2024★ 1 cited

Formation of Giant Clumps in High- Disc Galaxies by Compressive Turbulence

Nir Mandelker, Omry Ginzburg, Avishai Dekel +4

We address the formation of giant clumps in violently unstable gas-rich disc galaxies at cosmic noon. While these are commonly thought to originate from gravitational Toomre instab…

astro-ph.GA2024★ 1 cited

The Interplay between the IMF and Star Formation Efficiency through Radiative Feedback at High Stellar Surface Densities

Shyam H. Menon, Lachlan Lancaster, Blakesley Burkhart +3

The observed rest-UV luminosity function at cosmic dawn () measured by JWST revealed an excess of UV-luminous galaxies relative to many pre-launch theoretical predicti…

astro-ph.GA2024★ 8 cited

What drives the corpulence of galaxies? I. The formation of central compact dwarf galaxies in TNG50

Abhner P. De Almeida, Gary A. Mamon, Avishai Dekel +1

Nearby dwarf galaxies display a variety of effective radii (sizes) at a given stellar mass, suggesting different evolution scenarios according to their final "stellar" size. The TN…

astro-ph.GA2024★ 10 cited

Connection between galaxy morphology and dark-matter halo structure I: a running threshold for thin discs and size predictors from the dark sector

Jinning Liang, Fangzhou Jiang, Houjun Mo +5

We study the connection between galaxy morphology and host dark matter (DM) halo structure using cosmological simulations. Introducing a new kinematic decomposition scheme, we robu…

astro-ph.GA2024★ 20 cited

JWST/MIRI reveals the true number density of massive galaxies in the early Universe

Tao Wang, Hanwen Sun, Luwenjia Zhou +13

Early JWST studies reporting an unexpected abundance of massive galaxies at -- challenge galaxy formation models in the CDM framework. Previous stellar mass ($M_\st…