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20152023
most citedMassive Galaxies are Larger in Dense Environments: Environmental Dependence of Mass-Size Relation of Early-Type Galaxies

50 citations · 201 across the 17 of their papers we have counts for

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22 papers · 1 filter

astro-ph.GA2023★ 1 cited

BCG alignment with the Locations of Cluster Members and the Large Scale Structure out to 10 R

Rory Smith, Ho Seong Hwang, Katarina Kraljic +8

Using a sample of clusters, each with typically spectroscopically confirmed cluster members, we search for a signal of alignment between the Position Angle (PA) of…

astro-ph.GA2023

Galaxy Quenching with Mass Growth History of Galaxy Groups and Clusters: The Importance of Post-Processing

So-Myoung Park, Kyungwon Chun, Jihye Shin +5

We investigate the fraction of quenched satellite galaxies in host galaxy groups and clusters using TNG300 in the IllustrisTNG cosmological magnetohydrodynamical simulations. Simul…

astro-ph.GA2023★ 4 cited

Star formation history of mass-selected galaxies in the ELAIS-N1 Field

E. F. Ocran, M. Vaccari, J. M. Stil +3

We measure the specific star formation rates of \textit{K}-band selected galaxies from the ELAIS-N1 by stacking GMRT data at 610 MHz. We identify a sample of SFGs, spanning $\rm{0.…

astro-ph.GA2023★ 11 cited

Impact of Galaxy Mergers on Stellar Population Profiles of Early-type Galaxies

Yongmin Yoon, Jongwan Ko, Jae-Woo Kim

We study the impact of galaxy mergers on stellar population profiles/gradients of early-type galaxies (ETGs) using ETGs at in the Stripe 82 region of the Sloan Digital Sk…

astro-ph.GA2022★ 8 cited

Performance Assessment of the KASI-Deep Rolling Imaging Fast-optics Telescope pathfinder

Woowon Byun, Jongwan Ko, Yunjong Kim +14

In a CDM universe, most galaxies evolve by mergers and accretions, leaving faint and/or diffuse structures, such as tidal streams and stellar halos. Although these structures ar…

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…