activity
20122023
most citedCANDELS+3D-HST: compact SFGs at z~2-3, the progenitors of the first quiescent galaxies

181 citations · 1.1k across the 29 of their papers we have counts for

collaborators

30 papers

astro-ph.GA2023★ 6 cited

On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation

Ankit Singh, Changbom Park, Ena Choi +6

We use the Horizon Run 5 cosmological simulation to study the effect of galaxy intrinsic properties and the local environment on AGNs characterized by their threshold of the accret…

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…

physics.plasm-ph2022★ 15 cited

Mesoscopic transport in KSTAR plasmas: avalanches and the staircase

Minjun J. Choi, Jae-Min Kwon, Lei Qi +18

The self-organization is one of the most interesting phenomena in the non-equilibrium complex system, generating ordered structures of different sizes and durations. In tokamak pla…

astro-ph.GA2022

Simulating Jellyfish Galaxies: A Case Study for a Gas-Rich Dwarf Galaxy

Jaehyun Lee, Taysun Kimm, Jérémy Blaizot +5

We investigate the formation of jellyfish galaxies using radiation-hydrodynamic simulations of gas-rich dwarf galaxies with a multi-phase interstellar medium (ISM). We find that th…

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…

physics.plasm-ph2021★ 11 cited

Stochastic fluctuation and transport of tokamak edge plasmas with the resonant magnetic perturbation field

Minjun J. Choi, Jae-Min Kwon, Juhyung Kim +17

We present that a statistical method known as the Complexity-Entropy analysis is useful to characterize a state of plasma turbulence and flux in the resonant magnetic perturbation…

astro-ph.GA2020★ 40 cited

Dual Effects of Ram Pressure on Star Formation in Multi-phase Disk Galaxies with Strong Stellar Feedback

Jaehyun Lee, Taysun Kimm, Harley Katz +3

We investigate the impact of ram pressure stripping due to the intracluster medium (ICM) on star-forming disk galaxies with a multi-phase interstellar medium (ISM) maintained by st…

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★ 26 cited

The Dust-to-Gas Ratio and the Role of Radiation Pressure in Luminous, Obscured Quasars

Hyunsung D. Jun, Roberto J. Assef, Christopher M. Carroll +5

The absence of high Eddington ratio, obscured Active Galactic Nuclei (AGN) in local () samples of moderate luminosity AGN has generally been explained to result from…

astro-ph.GA2020★ 18 cited

Compact elliptical galaxies in different local environments: a mixture of galaxies with different origins?

Suk Kim, Hyunjin Jeong, Soo-Chang Rey +4

We present the stellar populations of 138 compact elliptical galaxies (cEs) in the redshift range of using the Sloan Digital Sky Survey (SDSS) DR12. Our cEs are divided…

astro-ph.GA2020★ 85 cited

The Horizon Run 5 Cosmological Hydrodynamic Simulation: Probing Galaxy Formation from Kilo- to Giga-parsec Scales

Jaehyun Lee, Jihye Shin, Owain N. Snaith +12

Horizon Run 5 (HR5) is a cosmological hydrodynamical simulation which captures the properties of the Universe on a Gpc scale while achieving a resolution of 1kpc. Inside the simula…

astro-ph.GA2018★ 22 cited

Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models

Rachel Asquith, Frazer R. Pearce, Omar Almaini +24

We present a comparison of the observed evolving galaxy stellar mass functions with the predictions of eight semi-analytic models and one halo occupation distribution model. While…

astro-ph.GA2018★ 20 cited

Wobbling galaxy spin axes in dense environments

Jaehyun Lee, Suk Kim, Hyunjin Jeong +7

The orientation of galaxy spin vectors within the large scale structure has been considered an important test of our understanding of structure formation. We investigate the angula…

astro-ph.GA2018★ 8 cited

Discovery of the kinematic alignment of early-type galaxies in the Virgo cluster

Suk Kim, Hyunjin Jeong, Jaehyun Lee +4

Using the kinematic position angles (PA_kin), an accurate indicator for the spin axis of a galaxy, obtained from the ATLAS3D integral-field-unit (IFU) spectroscopic data, we discov…

physics.plasm-ph2018★ 39 cited

Experimental evidence of the non-diffusive avalanche-like electron heat transport events and their dynamical interaction with the shear flow structure

Minjun J. Choi, Hogun Jhang, J. -M. Kwon +12

We present experimental observations suggesting that the non-diffusive avalanche-like events are a prevalent and universal process of the electron turbulent heat transport in tokam…

astro-ph.GA2017★ 31 cited

Cosmic CARNage I: on the calibration of galaxy formation models

Alexander Knebe, Frazer R. Pearce, Violeta Gonzalez-Perez +31

We present a comparison of nine galaxy formation models, eight semi-analytical and one halo occupation distribution model, run on the same underlying cold dark matter simulation (c…

astro-ph.GA2017★ 34 cited

nIFTy Cosmology: the clustering consistency of galaxy formation models

Arnau Pujol, Ramin A. Skibba, Enrique Gaztañaga +35

We present a clustering comparison of 12 galaxy formation models (including Semi-Analytic Models (SAMs) and Halo Occupation Distribution (HOD) models) all run on halo catalogues an…

astro-ph.GA2017★ 18 cited

Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass

Jaehyun Lee, Sukyoung K. Yi

Galaxy mass assembly is an end product of structure formation in the CDM cosmology. As an extension of Lee \& Yi (2013), we investigate the assembly history of stellar component…

astro-ph.GA2016★ 108 cited

The Preferential Tidal Stripping of Dark Matter versus Stars in Galaxies

Rory Smith, Hoseung Choi, Jaehyun Lee +3

Using high resolution hydrodynamical cosmological simulations, we conduct a comprehensive study of how tidal stripping removes dark matter and stars from galaxies. We find that dar…

astro-ph.GA2016★ 44 cited

Timing the evolution of quiescent and star-forming local galaxies

Camilla Pacifici, Sree Oh, Kyuseok Oh +2

Constraining the star formation histories (SFHs) of individual galaxies is crucial to understanding the mechanisms that regulate their evolution. Here, we combine multi-wavelength…

astro-ph.GA2015★ 22 cited

Demographics of Isolated Galaxies Along the Hubble Sequence

Hong-geun Khim, Jongwon Park, Seong-Woo Seo +3

Isolated galaxies in low-density regions are significant in the sense that they are least affected by the hierarchical pattern of galaxy growth, and interactions with perturbers, a…

astro-ph.GA2015

nIFTy Cosmology: Comparison of Galaxy Formation Models

Alexander Knebe, Frazer R. Pearce, Peter A. Thomas +33

We present a comparison of 14 galaxy formation models: 12 different semi-analytical models and 2 halo-occupation distribution models for galaxy formation based upon the same cosmol…

nucl-th2014

Stiffer EoS for Compact Star with New Scaling Law

Kyungmin Kim, T. T. S. Kuo, Hyun Kyu Lee +2

We present in this paper a simple and unequivocal prediction on the deformation of the compact star, that will be measured in gravity waves, with an EoS obtained in renormailzation…

astro-ph.GA2014★ 36 cited

Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model

Jaehyun Lee, Sukyoung K. Yi, Pascal J. Elahi +13

A halo merger tree forms the essential backbone of a semi-analytic model for galaxy formation and evolution. Recent studies have pointed out that extracting merger trees from numer…