Showing 1–20 of 154 results
/ Date/ Name
Feb 11, 2019Black versus Dark: Rapid Growth of Supermassive Black Holes in Dark Matter Halos at z ~ 6Mar 11, 2004Large Cosmic Variance in the Clustering Properties of Lyman Alpha Emitters at z~5Apr 18, 2005Number Density of Bright Lyman-Break Galaxies at z~6 in the Subaru Deep FieldFeb 28, 2006Ly Alpha Emitters at z=5.7 in the Subaru Deep FieldJul 13, 2010Stellar Populations of Lyman-alpha Emitters at z=4.86: A Comparison to $z\sim5$ LBGsFeb 1, 2012Dust Attenuation and H-alpha Star Formation Rates of z~0.5 GalaxiesDec 17, 2011The First Systematic Survey for Lyman Alpha Emitters at z=7.3 with Red-sensitive Subaru/Suprime-CamAug 28, 2010Lyman Alpha Emitters at z=7 in the Subaru/XMM-Newton Deep Survey Field: Photometric Candidates and Luminosity FunctionJul 17, 2010Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation ModelsApr 12, 2011Completing the Census of Ly-alpha Emitters at the Reionization EpochJun 11, 2012Gas Motion Study of Lya Emitters at z~2 Using UV and Optical Spectral LinesMar 6, 2012Discovery of a protocluster at z~6Nov 13, 2009Stellar Populations of Lyman Alpha Emitters at z = 3 - 4 Based on Deep Large Area Surveys in the Subaru-SXDS/UKIDSS-UDS FieldDec 15, 2009Panoramic H-alpha and mid-infrared mapping of star formation in a z=0.8 clusterNov 2, 2022ALMA Observations for CO Emission from Luminous Lyman-break Galaxies at $z=6.0293$-$6.2037$Sep 16, 2008Mapping dusty star formation in and around a cluster at z=0.81 by wide-field imaging with AKARIMay 23, 2022MUSUBI (MegaCam Ultra-deep Survey: $u^\ast$-Band Imaging)-Data for the COSMOS and SXDS FieldsApr 24, 2014Accelerated Evolution of Ly$α$ Luminosity Function at $\textit{z} \gtrsim 7$ Revealed by the Subaru Ultra-Deep Survey for Ly$α$ Emitters at $\textit{z}=7.3$Aug 29, 2014Hubble Frontier Fields First Complete Cluster Data: Faint Galaxies at $z\sim 5-10$ for UV Luminosity Functions and Cosmic ReionizationFeb 24, 2020A Systematic Search for Galaxy Proto-Cluster Cores at $z\sim 2$