Showing 1–20 of 46 results
/ Date/ Name
Aug 30, 2017GOLDRUSH. III. A Systematic Search of Protoclusters at $z\sim4$ Based on the $>100\,\mathrm{deg^2}$ AreaMar 6, 2012Discovery of a protocluster at z~6Apr 24, 2024Galaxy properties from the outskirts to the core of a protocluster at z=3.699Oct 12, 2023An enhanced abundance of bright galaxies in protocluster candidates at z~3-5Dec 3, 2019Discovery of Protoclusters at z~3.7 & 4.9: Embedded in Primordial SuperclustersMay 4, 2016A Systematic Survey of Protoclusters at $z\sim3\mathrm{-}6$ in the CFHTLS Deep FieldsJul 7, 2014A First Site of Galaxy Cluster Formation: Complete Spectroscopy of a Protocluster at $z=6.01$Jul 6, 2020The UV Luminosity Function of Protocluster Galaxies at $z\sim4$: the Bright-end Excess and the Enhanced Star Formation Rate DensityJan 22, 2019Environmental impacts on molecular gas in protocluster galaxies at z~2Nov 30, 2023Nature vs. Nurture: Revisiting the environmental impact on star formation activities of galaxiesNov 21, 2019Planck far-infrared detection of Hyper Suprime-Cam protoclusters at $\bf z\sim4$: hidden AGN and star formation activityFeb 12, 2021Accelerated galaxy growth and environmental quenching in a protocluster at z=3.24Nov 18, 2024Mining for Protoclusters at $z\sim4$ from Photometric Datasets with Deep LearningDec 20, 2016The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep FieldsJul 29, 2024Environments around quasars at $z\sim$3 revealed by wide-field imaging with Subaru HSC and CFHTApr 22, 2026The Evolution of the SFR-M_* relation at 0.1<z<4: Environmental and Morphological DependenciesJan 20, 2022Cool outflows in MaNGA: a systematic study and comparison to the warm phaseAug 31, 2022A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). IX. The Most Overdense Region at z~5 Inhabited by a Massive Radio GalaxyJul 14, 2020A detailed study of massive galaxies in a protocluster at z=3.13May 15, 2019How Do Galaxies trace a large scale structure?: A case study around a massive protocluster at $z=3.13$