Showing 1–20 of 74 results
/ Date/ Name
Aug 20, 2020Revisiting the Gas Kinematics in SSA22 Lyman-$α$ Blob 1 with Radiative Transfer Modeling in a Multiphase, Clumpy MediumApr 21, 2021Where Outflows Meet Inflows: Gas Kinematics in SSA22 Lyman-$α$ Blob 2 Decoded by Advanced Radiative Transfer ModellingMar 6, 2026The Prevalence of Turbulence-Regulated Multiphase Galactic Winds in Star-Forming GalaxiesNov 5, 2021Deciphering the Lyman-$α$ Emission Line: Towards the Understanding of Galactic Properties Extracted from Ly$α$ Spectra via Radiative Transfer ModelingMar 2, 2020A polarization quantum key distribution scheme based on phase matchingNov 28, 2014Design of a 10 MeV normal conducting CW proton linac based on equidistant multi-gap CH cavitiesNov 11, 2024High-Frequency Enhanced Hybrid Neural Representation for Video CompressionMar 12, 2026BLUEPRINT: Blue-dominant Lyman-alpha (Ly$α$) emission as an evidence of gas inflow in ultra-low-mass galaxies at z = 3Jun 19, 2023ALPACA: A New Semi-Analytic Model for Metal Absorption Lines Emerging from Clumpy Galactic EnvironmentsMay 26, 2020SN2019dge: a Helium-rich Ultra-Stripped Envelope SupernovaApr 20, 2021The KBSS-KCWI Survey: The connection between extended Ly$α$ halos and galaxy azimuthal angle at $z\sim 2-3$Mar 7, 2017Focusing properties of discrete RF quadrupoleJun 5, 2019The Evolution of the Interstellar Medium in Post-Starburst GalaxiesSep 5, 2019On the Survival of Cool Clouds in the Circum-Galactic MediumOct 15, 2024Synergistic Radiative Transfer Modeling of MgII and Lyα Emission in Multiphase, Clumpy Galactic Environments: Application to Low-Redshift Lyman Continuum LeakersOct 19, 2016The focusing properties of both normal and superconducting low energy CW proton LinacsApr 9, 2025FANeRV: Frequency Separation and Augmentation based Neural Representation for VideoDec 30, 2013A CW superconducting linac as the proton driver for a medium baseline neutrino beam in ChinaApr 30, 2018Extreme [OIII] Emitters at z $\sim$ 0.5Mar 6, 2026Kinematically Coherent Multiphase Galactic Winds in Star-Forming Galaxies Revealed by Unified Radiative Transfer Modeling of UV Emission and Absorption Lines