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20162024
most citedIntroducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time

229 citations · 1k across the 16 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.GA2020★ 20 cited

Star-Gas Misalignment in Galaxies: II. Origins Found from the Horizon-AGN Simulation

Donghyeon J. Khim, Sukyoung K. Yi, Christophe Pichon +5

There have been many studies aiming to reveal the origins of the star-gas misalignment found in galaxies, but there still is a lack of understanding of the contribution from each f…

astro-ph.GA2020★ 12 cited

YZiCS: On the Mass Segregation of Galaxies in Clusters

Seonwoo Kim, Emanuele Contini, Hoseung Choi +5

Mass segregation, a tendency of more massive galaxies being distributed closer to the cluster center, is naturally expected from dynamical friction, but its presence is still contr…

astro-ph.GA2020★ 42 cited

Exploring the origin of thick disks using the NewHorizon and Galactica simulations

Minjung J. Park, Sukyoung K. Yi, Sebastien Peirani +8

Ever since a thick disk was proposed to explain the vertical distribution of the Milky Way disk stars, its origin has been a recurrent question. We aim to answer this question by i…

astro-ph.GA2020★ 229 cited

Introducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time

Yohan Dubois, Ricarda Beckmann, Frédéric Bournaud +13

Hydrodynamical cosmological simulations are increasing their level of realism by considering more physical processes and having greater resolution or larger statistics. However, us…

astro-ph.GA2020★ 73 cited

The role of mergers and interactions in driving the evolution of dwarf galaxies over cosmic time

G. Martin, R. A. Jackson, S. Kaviraj +9

Dwarf galaxies (M*<10^9 Msun) are key drivers of mass assembly in high mass galaxies, but relatively little is understood about the assembly of dwarf galaxies themselves. Using the…

astro-ph.GA2020★ 52 cited

YZiCS: Unveiling Quenching History of Cluster Galaxies Using Phase-space Analysis

Jinsu Rhee, Rory Smith, Hoseung Choi +4

We used the time since infall (TSI) of galaxies, obtained from the Yonsei Zoom-in Cluster Simulation, and the star formation rate (SFR) from the Sloan Digital Sky Survey (SDSS) Dat…