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The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at
Haruka Kusakabe, Kazuhiro Shimasaku, Masami Ouchi +7
We present average stellar population properties and dark matter halo masses of \lya emitters (LAEs) from SED fitting and clustering analysis, respectively, using $\sime…
SILVERRUSH. IV. Ly Luminosity Functions at and Studied with 1,300 LAEs on the deg Sky
Akira Konno, Masami Ouchi, Takatoshi Shibuya +18
We present the Ly luminosity functions (LFs) at 5.7 and 6.6 derived from a new large sample of 1,266 Ly emitters (LAEs) identified in total areas of 14 and 21 deg, re…
SILVERRUSH. III. Deep Optical and Near-Infrared Spectroscopy for Lya and UV-Nebular Lines of Bright Lya Emitters at z=6-7
Takatoshi Shibuya, Masami Ouchi, Yuichi Harikane +23
We present Lya and UV-nebular emission line properties of bright Lya emitters (LAEs) at z=6-7 with a luminosity of log L_Lya/[erg s-1] = 43-44 identified in the 21-deg2 area of the…
SILVERRUSH. II. First Catalogs and Properties of ~2,000 Lya Emitters and Blobs at z~6-7 Identified over the 14-21 deg2 Sky
Takatoshi Shibuya, Masami Ouchi, Akira Konno +19
We present an unprecedentedly large catalog consisting of 2,230 > L* Lya emitters (LAEs) at z=5.7 and 6.6 on the 13.8 and 21.2 deg2 sky, respectively, that are identified by the SI…
Systematic Identification of LAEs for Visible Exploration and Reionization Research Using Subaru HSC (SILVERRUSH). I. Program Strategy and Clustering Properties of ~2,000 Lya Emitters at z=6-7 over the 0.3-0.5 Gpc Survey Area
Masami Ouchi, Yuichi Harikane, Takatoshi Shibuya +17
We present the SILVERRUSH program strategy and clustering properties investigated with Ly emitters at and found in the early data of the Hyper Suprime…
GOLDRUSH. II. Clustering of Galaxies at Revealed with the Half-Million Dropouts Over the 100 deg Area Corresponding to 1 Gpc
Yuichi Harikane, Masami Ouchi, Yoshiaki Ono +15
We present clustering properties from 579,492 Lyman break galaxies (LBGs) at z~4-6 over the 100 deg^2 sky (corresponding to a 1.4 Gpc^3 volume) identified in early data of the Hype…