Showing 1–20 of 24 results
/ Date/ Name
Dec 17, 2009A wide-field photometric survey for extratidal tails around five metal-poor globular clusters in the Galactic haloOct 7, 2014Tidal stripping stellar substructures around four metal-poor globular clusters in the Galactic bulgeAug 24, 2020Extra-tidal stars and chemical abundance properties of two metal-poor globular clusters M53 (NGC 5024) and NGC 5053Mar 20, 2024Is the RSGC4 (Alicante 8) cluster a real star cluster?: Peculiar radial velocities of red supergiant starsOct 19, 2022Red supergiant stars in IC 1613 and metallicity-dependent mixing length in the evolutionary modelNov 9, 2017Evolutionary models of red supergiants: Evidence for a metallicity-dependent mixing length and implications for Type IIP supernova progenitorsJul 29, 2022Performance Assessment of the KASI-Deep Rolling Imaging Fast-optics Telescope pathfinderAug 28, 2023The SN 2023ixf Progenitor in M101: II. PropertiesDec 4, 2014Low-resolution Spectroscopy for the Globular Clusters with Signs of Supernova Enrichment: M22, NGC 1851 and NGC 288Dec 22, 2025K-DRIFT Science Theme: Illuminating the Next Era of Galaxy Cluster ScienceOct 28, 2024Two stellar populations with different metallicities in the low-mass globular cluster Gran 5Jan 6, 2026A New Collision Avoidance Fiber Assignment Algorithm for Robotic Fiber Positioners in Multi-Object SpectroscopyFeb 9, 2026K-DRIFT Science Theme: Galaxies in the Faint UniverseJun 19, 2023The SN 2023ixf Progenitor in M101: I. Infrared VariabilityNov 14, 2023Chemical homogeneity of wide binary system: An approach from Near-Infrared spectroscopyDec 20, 2024Dynamical Evolution of Substructured Star Clusters at 3 kpc from the Galactic CenterMay 23, 2012Near-infrared properties of asymptotic giant branch stars in nearby dwarf elliptical Galaxy NGC 205Oct 25, 2025K-DRIFT: Unveiling New Imagery of the Hidden UniverseJan 22, 2026K-DRIFT Science Theme: Galactic Cirrus Clouds and Circumgalactic MediumMar 9, 2026K-DRIFT Science Theme: New Theoretical Framework Using the Galaxy Replacement Technique for LSB studies