most citedThe physical origin for spatially large scatter of IGM opacity at the end of reionization: the IGM Ly opacity-galaxy density relation

18 citations · 30 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.GA202352 cited

COSMOS2020: Discovery of a protocluster of massive quiescent galaxies at

Kei Ito, Masayuki Tanaka, Francesco Valentino +9

Protoclusters of galaxies have been found in the last quarter century. However, most of them have been found through the overdensity of star-forming galaxies, and there had been no…

astro-ph.GA2023

MAMMOTH-Subaru V. Effects of Cosmic Variance on Ly Luminosity Functions at

Ke Ma, Haibin Zhang, Zheng Cai +8

Cosmic variance introduces significant uncertainties into galaxy number density properties when surveying the high-z Universe with a small volume, such uncertainties produce the fi…

astro-ph.GA20231 cited

MAMMOTH-Subaru III. Ly Halo Extended to kpc Identified by Stacking Ly Emitters at

Haibin Zhang, Zheng Cai, Yongming Liang +8

In this paper, we present a Ly halo extended to kpc identified by stacking Ly emitters at . We carry out imaging observations and data reduct…

astro-ph.GA202218 cited

The physical origin for spatially large scatter of IGM opacity at the end of reionization: the IGM Ly opacity-galaxy density relation

Rikako Ishimoto, Nobunari Kashikawa, Daichi Kashino +9

The large opacity fluctuations in the Ly forest may indicate inhomogeneous progress of reionization. To explain the observed large scatter of the effective Ly optic…

astro-ph.GA202112 cited

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed by High-z Radio Galaxies at z~4

Hisakazu Uchiyama, Takuji Yamashita, Jun Toshikawa +13

We present the environmental properties around high- radio galaxies (HzRGs) at , which have been poorly investigated because of their rarity. We use the largest samples…