activity
20242026
collaborators

9 papers

astro-ph.CO2026

New classification method for the dynamical state of galaxy clusters with a Gaussian mixture model

Hyowon Kim, Marco Canducci, Rory Smith +5

Galaxy clusters are the largest gravitationally bound systems, and they continue their growth through mergers in a hierarchical ΛCDM Universe. Therefore, we can describe the merge…

astro-ph.GA2026

K-DRIFT Science Theme: Galaxies in the Faint Universe

Woowon Byun, Yongmin Yoon, Jongwan Ko +17

Low-surface-brightness (LSB) structures serve as evidence of the intricate mass assembly of galaxies, and dedicatedly studying them promises to give us profound insights into the e…

astro-ph.GA2026

Convolutional Neural Networks for classifying galaxy mergers: Can faint tidal features aid in classifying mergers?

Yeonkyung Lee, Hyunmi Song, Jihye Shin +3

Identifying mergers from observational data has been a crucial aspect of studying galaxy evolution and formation. Tidal features, typically fainter than 26

astro-ph.GA2026

K-DRIFT Science Theme: Galactic Cirrus Clouds and Circumgalactic Medium

Kwang-il Seon, Jaehyun Lee, Jongwan Ko +8

In this paper, we review the extended halo material and the circumgalactic medium (CGM), including both dust and gas, and discuss promising science cases that could be realized usi…

astro-ph.GA2025

K-DRIFT Science Theme: Illuminating the Next Era of Galaxy Cluster Science

Jaewon Yoo, Kyungwon Chun, Jongwan Ko +13

The KASI Deep Rolling Imaging Fast Telescope (K-DRIFT) is a pioneering instrument designed to explore low-surface-brightness (LSB) phenomena. This white paper presents a compelling…

astro-ph.GA2025

Direct observational evidence that higher-luminosity type 1 active galactic nuclei are most commonly triggered by galaxy mergers

Yongmin Yoon, Yongjung Kim, Dohyeong Kim +2

We examine the connection between galaxy mergers and the triggering of active galactic nuclei (AGNs) using a sample of 614 type 1 AGNs at , along with a control sample of i…