Abstract The Cosmic Evolution Survey (COSMOS) is designed to probe the correlated
evolution of galaxies, star formation, active galactic nuclei (AGNs), and dark matter (DM) with …

The Universe's dark ages end with the formation of the first generation of galaxies. These
objects start emitting ultraviolet radiation that carves out ionized regions around them. After a …

We present new measurements of rest-UV luminosity functions and angular correlation
functions from 4,100,221 galaxies at z∼ 2–7 identified in the Subaru/Hyper Suprime-Cam …

We study the UV luminosity functions (LFs) at z∼ 4, 5, 6, and 7 based on the deep large-
area optical images taken by the Hyper Suprime-Cam (HSC) Subaru Strategic Program …

Faint Lyα emitters become increasingly rarer toward the reionization epoch (z∼ 6–7).
However, observations from a very large (∼ 5 deg 2) Lyα narrow-band survey at z= 6.6 …

We present the SILVERRUSH program strategy and clustering properties investigated
with∼ 2000 Lyα emitters (LAEs) at z= 5.7 and 6.6 found in the early data of the Hyper …

We present the Lyα luminosity function (LF), clustering measurements, and Lyα line profiles
based on the largest sample to date of 207 Lyα emitters (LAEs) at z= 6.6 on the 1 deg 2 sky …

We present the Lyα luminosity functions (LFs) at z= 5.7 and 6.6 derived from a new large
sample of 1266 Lyα emitters (LAEs) identified in total areas of 14 and 21 deg2, respectively …

We present luminosity functions (LFs) and various properties of Lyα emitters (LAEs) at z=
3.1, 3.7, and 5.7, in a 1 deg 2 sky of the Subaru/XMM–Newton Deep Survey (SXDS) Field …

We present deep optical imaging observations of 2 square degree area, covered by the
Cosmic Evolution Survey (COSMOS), made by the prime-focus camera (Supreme-Cam) on …