activity
20242026
most citedGalaxies with grains: unraveling dust evolution and extinction curves with hydrodynamical simulations

29 citations · 36 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

Kinematic scaling of thin and thick discs from SAMI to NewHorizon

Sree Oh, J. K. Jang, Giulia Santucci +8

We revisit the relation between disc stellar mass and disc velocity dispersion (M_*-σ_e) and extend it to thin and thick subcomponents using orbit-based dynamical models of 161 SAM…

astro-ph.GA2026

Black Hole Occupation Fraction: Dependence on Black Hole Mass Threshold, Environment, Resolution and Redshift

Emanuele Contini, J. K. Jang, Jinsu Rhee +2

We take advantage of the state-of-the-art semi-analytic model \texttt{FEGA25} \citep{contini2025}, run on merger trees extracted from three dark matter-only cosmological simulation…

astro-ph.GA2025★ 2 cited

On the Origin of Intracluster Light based on the High-resolution Simulation, NewCluster

Seyoung Jeon, Emanuele Contini, San Han +11

Intracluster light (ICL) is a key component of galaxy clusters, with the potential to trace their dynamical assembly histories and the underlying dark matter distribution. Despite…

astro-ph.GA2025

On the Origin of Gas-stripping of Galaxies in Group Environments

Jinsu Rhee, Christophe Pichon, Yohan Dubois +12

We investigate how low-mass group environments () influence the gas content of their satellite galaxies with using…

astro-ph.GA2025

How Dust Models Shape High-z Galaxy Morphology: Insights from the NewCluster Simulation

Gyeong-Hwan Byun, J. K. Jang, Zachary P. Scofield +10

Dust plays a pivotal role in shaping the observed morphology of galaxies. While traditional cosmological simulations often assume a fixed dust-to-gas (DTG) or dust-to-metal (DTM) m…

astro-ph.GA2025★ 5 cited

Introducing NewCluster: the first half of the history of a high-resolution cluster simulation

San Han, Sukyoung K. Yi, Yohan Dubois +8

We introduce NewCluster, a new high-resolution cluster simulation designed to serve as the massive halo counterpart of the modern cosmological galaxy evolution framework. The zoom-…

astro-ph.GA2024

Exploring lenticular galaxy formation in field environments using NewHorizon: evidence for counter-rotating gas accretion as a formation channel

Seongbong Han, J. K. Jang, Emanuele Contini +9

The formation pathways of lenticular galaxies (S0s) in field environments remain a matter of debate. We utilize the cosmological hydrodynamic simulation, NewHorizon, to investigate…

astro-ph.GA2024

On the Origin of Star Formation Quenching of Galaxies in Group Environments using the NewHorizon simulation

Jinsu Rhee, Sukyoung K. Yi, Jongwan Ko +8

We study star formation (SF) quenching of satellite galaxies with within two low-mass groups ( and ) using t…

astro-ph.GA2024

Formation pathways of the compact stellar systems

J. K. Jang, Sukyoung K. Yi, Soo-Chang Rey +6

The formation pathways of compact stellar systems (CSSs) are still under debate. We utilize the \NH\ simulation to investigate the origins of such objects in the field environment.…

astro-ph.GA2024★ 29 cited

Galaxies with grains: unraveling dust evolution and extinction curves with hydrodynamical simulations

Yohan Dubois, Francisco Rodríguez Montero, Corentin Guerra +6

We introduce a model for dust evolution in the RAMSES code for simulations of galaxies with a resolved multiphase interstellar medium. Dust is modelled as a fluid transported with…