activity
20232026
most citedRIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars

36 citations · 230 across the 36 of their papers we have counts for

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Showing 2025Show all

16 papers · 1 filter

astro-ph.GA2025★ 1 cited

RIGEL: Feedback-regulated cloud-scale star formation efficiency in a simulated dwarf galaxy merger

Yunwei Deng, Hui Li, Federico Marinacci +5

Major mergers of galaxies are likely to trigger bursty star formation activities. The accumulation of dense gas and the boost of star formation efficiency (SFE) are considered to b…

astro-ph.GA2025

Modelling the nebular emission of galaxies across cosmic time with COLT

William McClymont, Aaron Smith, Sandro Tacchella

Extragalactic nebular emission has long been a workhorse probe of the processes driving galaxy evolution, but the richness of JWST spectroscopy has shifted the bottleneck from data…

astro-ph.GA2025

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift

Alex M. Garcia, Paul Torrey, Aniket Bhagwat +22

The distribution of gas-phase metals within galaxies encodes the impact of stellar feedback on galactic evolution. At high-redshift, when galaxies are rapidly assembling, feedback-…

astro-ph.GA2025★ 2 cited

The THESAN-ZOOM project: The Hidden Neighbours of OI Absorbers during Reionization

Giulia Pruto, Laura Keating, Rahul Kannan +9

Metal absorbers represent a powerful probe of galaxy feedback and reionization, as highlighted by both observational and theoretical results showing an increased abundance of low-i…

astro-ph.GA2025★ 1 cited

The Entangling of Supernova Feedback Impacts with Coarsening Simulation Resolution

Eric Zhang, Laura V. Sales, Thales A. Gutcke +11

It is often understood that supernova (SN) feedback in galaxies is responsible for regulating star formation (SF) and generating gaseous outflows. However, a detailed look at the s…

astro-ph.GA2025★ 3 cited

High-redshift AGN population in radiation-hydrodynamics simulations

Teodora-Elena Bulichi, Oliver Zier, Aaron Smith +7

High-redshift active galactic nuclei (AGN) have long been recognized as key probes of early black hole growth and galaxy evolution. However, modeling this population remains diffic…

astro-ph.GA2025★ 5 cited

The THESAN-ZOOM project: Mystery N/O more -- uncovering the origin of peculiar chemical abundances and a not-so-fundamental metallicity relation at

William McClymont, Sandro Tacchella, Aaron Smith +15

We present an analysis of metallicities and chemical abundances at in the THESAN-ZOOM simulations. We find that smoothly curved gas-phase and stellar mass-metallicity rela…

astro-ph.GA2025★ 7 cited

Overmassive black holes in the early Universe can be explained by gas-rich, dark matter-dominated galaxies

William McClymont, Sandro Tacchella, Xihan Ji +12

JWST has revealed the apparent evolution of the black hole (BH)-stellar mass (-$M_\rm{\ast}$) relation in the early Universe, while remaining consistent with the BH-…

astro-ph.GA2025★ 7 cited

The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts

Zihao Wang, Xuejian Shen, Mark Vogelsberger +12

Star formation in galaxies is inherently complex, involving the interplay of physical processes over a hierarchy of spatial scales. In this work, we investigate the connection betw…

astro-ph.GA2025★ 4 cited

JWST ASPIRE: How Did Galaxies Complete Reionization? Evidence for Excess IGM Transmission around Emitters during Reionization

Koki Kakiichi, Xiangyu Jin, Feige Wang +23

The spatial correlation between galaxies and the Ly forest provides insights into how galaxies reionized the Universe. Here, we present initial results on the spatial cross-corr…

astro-ph.GA2025★ 8 cited

The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies

Xuejian Shen, Rahul Kannan, Ewald Puchwein +10

Recent JWST observations hint at unexpectedly intense cosmic star-formation in the early Universe, often attributed to enhanced star-formation efficiencies (SFEs). Here, we analyze…

astro-ph.GA2025★ 14 cited

The THESAN-ZOOM project: central starbursts and inside-out quenching govern galaxy sizes in the early Universe

William McClymont, Sandro Tacchella, Aaron Smith +9

We explore the evolution of galaxy sizes at high redshift () using the high-resolution THESAN-ZOOM radiation-hydrodynamics simulations, focusing on the mass range of $1…

astro-ph.GA2025★ 13 cited

The THESAN-ZOOM project: Population III star formation continues until the end of reionization

Oliver Zier, Rahul Kannan, Aaron Smith +8

Population III (Pop III) stars are the first stars in the Universe, forming from pristine, metal-free gas and marking the end of the cosmic dark ages. Their formation rate is expec…

astro-ph.GA2025★ 2 cited

The THESAN-ZOOM project: Long-term imprints of external reionization on galaxy evolution

Oliver Zier, Rahul Kannan, Aaron Smith +8

We investigate the impact of ionizing external ultraviolet (UV) radiation on low-mass haloes () at high redshift using baryonic resolution zoom-…

astro-ph.GA2025★ 25 cited

The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence

William McClymont, Sandro Tacchella, Aaron Smith +10

Characterizing the evolution of the star-forming main sequence (SFMS) at high redshift is crucial to contextualize the observed extreme properties of galaxies in the early Universe…

astro-ph.GA2025★ 25 cited

Introducing the THESAN-ZOOM project: radiation-hydrodynamic simulations of high-redshift galaxies with a multi-phase interstellar medium

Rahul Kannan, Ewald Puchwein, Aaron Smith +11

We introduce the THESAN-ZOOM project, a comprehensive suite of high-resolution zoom-in simulations of high-redshift () galaxies selected from the THESAN simulation volume…