Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …

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 …

Photometric redshifts are a key component of many science objectives in the Hyper Suprime-
Cam Subaru Strategic Program (HSC-SSP). In this paper, we describe and compare the …

We present Keck–MOSFIRE H and K spectra for a sample of 24 candidate quiescent
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …

We present the ancillary data and basic physical measurements for the galaxies in the
ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey—the first large …

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 …

We study the efficiency of galactic feedback in the early Universe by stacking the [C II] 158
μm emission in a large sample of normal star-forming galaxies at 4< z< 6 from the ALMA …

We present a" super-deblended" far-infrared (FIR) to (sub) millimeter photometric catalog in
the Cosmic Evolution Survey (COSMOS), prepared with the method recently developed by …

We study the composition of the faint radio population selected from the Karl G. Jansky Very
Large Array Cosmic Evolution Survey (VLA-COSMOS) 3 GHz Large Project, which is a radio …

We examine the behaviour of the infrared-radio correlation (IRRC) over the range 0< z≲ 6
using new, highly sensitive 3 GHz observations with the Karl G. Jansky Very Large Array …