Showing 1–20 of 21 results
/ Date/ Name
Jun 19, 2019Cosmological Simulations of Satellites around Isolated Dwarf GalaxiesMay 13, 2024Formation channels of the diffuse lights in the groups and clusters over timeSep 26, 2025The Role of Pre-Processing in Tidal Feature Formation within Galaxy ClustersDec 22, 2025K-DRIFT Science Theme: Illuminating the Next Era of Galaxy Cluster ScienceOct 18, 2021The Galaxy Replacement Technique (GRT): a New Approach to Study Tidal Stripping and Formation of Intracluster Light in a Cosmological ContextMar 9, 2026K-DRIFT Science Theme: New Theoretical Framework Using the Galaxy Replacement Technique for LSB studiesDec 5, 2022The formation of the brightest cluster galaxy and intracluster light in cosmological N-body simulations with the Galaxy Replacement TechniqueJul 11, 2023Galaxy Quenching with Mass Growth History of Galaxy Groups and Clusters: The Importance of Post-ProcessingDec 10, 2019The Gas Accretion History of Low Mass Halos within the Cosmic Web from Cosmological SimulationsDec 2, 2025Direct observational evidence that higher-luminosity type 1 active galactic nuclei are most commonly triggered by galaxy mergersMay 17, 2022Comparison of spatial distributions of Intracluster light and Dark MatterFeb 9, 2026K-DRIFT Science Theme: Galaxies in the Faint UniverseMay 10, 2024New observational recipes for measuring dynamical state of galaxy clustersDec 20, 2024Dynamical Evolution of Substructured Star Clusters at 3 kpc from the Galactic CenterOct 25, 2025K-DRIFT: Unveiling New Imagery of the Hidden UniverseJan 22, 2026K-DRIFT Science Theme: Galactic Cirrus Clouds and Circumgalactic MediumOct 27, 2022Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular ClustersApr 28, 2017Hydrodynamic simulations of the central molecular zone with realistic Galactic potentialFeb 3, 2026Convolutional Neural Networks for classifying galaxy mergers: Can faint tidal features aid in classifying mergers?Apr 4, 2024Shell-type Tidal Features Are More Frequently Detected in Slowly Rotating Early-type Galaxies than Stream- and Tail-type Features