activity
20082024
most citedThe Horizon Run 5 Cosmological Hydrodynamic Simulation: Probing Galaxy Formation from Kilo- to Giga-parsec Scales

85 citations · 654 across the 40 of their papers we have counts for

collaborators
Showing 2022Show all

11 papers · 1 filter

astro-ph.GA2022★ 21 cited

The formation of the brightest cluster galaxy and intracluster light in cosmological N-body simulations with the Galaxy Replacement Technique

Kyungwon Chun, Jihye Shin, Rory Smith +2

We investigate the formation channels of the intracluster light (ICL) and the brightest cluster galaxy (BCG) in clusters at . For this, we perform multi-resolution cosmologica…

astro-ph.GA2022★ 16 cited

Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function

Juhan Kim, Jaehyun Lee, Clotilde Laigle +8

We investigate the impact of the surface brightness (SB) limit on the galaxy stellar mass functions (GSMFs) using mock surveys generated from the Horizon Run 5 (HR5) simulation. We…

astro-ph.GA2022★ 2 cited

Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular Clusters

So-Myoung Park, Jihye Shin, Rory Smith +1

We investigate the properties of globular clusters in a galaxy cluster, using the particle tagging method with a semi-analytical approach in a cosmological context. We assume globu…

astro-ph.GA2022★ 17 cited

The First Fall is the Hardest: The Importance of Peculiar Galaxy Dynamics at Infall Time for Tidal Stripping Acting at the Centers of Groups and Clusters

Rory Smith, Paula Calderon-Castillo, Jihye Shin +2

Using dark matter only N-body cosmological simulations, we measure the pericentre distance of dark matter halos on their first infall into group and cluster halos. We find that the…

astro-ph.CO2022★ 11 cited

Unexpected dancing partners: Tracing the coherence between the spin and motion of dark matter halos

Yigon Kim, Rory Smith, Jihye Shin

A recent study conducted using CALIFA survey data (Lee et al, 2019b) has found that the orbital motions of neighbor galaxies are coherent with the spin direction of a target galaxy…

astro-ph.GA2022★ 27 cited

A New Method to Constrain the Appearance and Disappearance of Observed Jellyfish Galaxy Tails

Rory Smith, Jong-Ho Shinn, Stephanie Tonnesen +11

We present a new approach to observationally constrain where the tails of Jellyfish (JF) galaxies in groups and clusters first appear and how long they remain visible with respect…

astro-ph.GA2022★ 18 cited

Spatial distribution of dark matter in and around galaxy clusters traced by galaxies, gas and intracluster stars in a simulated universe

Jihye Shin, Jong Chul Lee, Ho Seong Hwang +5

To understand how well galaxies, gas and intracluster stars trace dark matter in and around galaxy clusters, we use the IllustrisTNG cosmological hydrodynamical simulation and comp…

astro-ph.GA2022★ 25 cited

Comparison of spatial distributions of Intracluster light and Dark Matter

Jaewon Yoo, Jongwan Ko, Cristiano G. Sabiu +7

In a galaxy cluster, the relative spatial distributions of dark matter, member galaxies, gas, and intracluster light (ICL) may connote their mutual interactions over the cluster ev…

astro-ph.GA2022★ 4 cited

Is Abell 2261 a fossil galaxy cluster in a transitional dynamical state?

Hyowon Kim, Jongwan Ko, Rory Smith +5

Abell 2261 (A2661) is a well-studied fossil cluster, but previous studies give contradictory results on its dynamical states, such as its X-ray central entropy and magnitude gap. T…

astro-ph.GA2022★ 33 cited

Formation and Morphology of the First Galaxies in the Cosmic Morning

Changbom Park, Jaehyun Lee, Juhan Kim +8

We investigate the formation and morphological evolution of the first galaxies in the cosmic morning () using the Horizon Run 5 (HR5) simulation. For galaxi…

astro-ph.CO2022★ 15 cited

Tracking Halo Orbits and Their Mass Evolution around Large-scale Filaments

Hannah Jhee, Hyunmi Song, Rory Smith +3

We have explored the dynamical and mass evolution of halos driven by large-scale filaments using a dark matter-only cosmological simulation with the help of a phase-space analysis.…