The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …

Hydrogen Lyman-α (Lyα) emission has been one of the major observational probes for the
high-redshift Universe since the first discoveries of high-z Lyα-emitting galaxies in the late …

ABSTRACT A very simple physical model of galaxies is one in which the formation of stars is
instantaneously regulated by the mass of gas in a reservoir with mass loss scaling with the …

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 a systematic study for ionization state of inter-stellar medium in galaxies at z= 0–
with∼ 140 000 Sloan Digital Sky Survey (SDSS) galaxies and 108 intermediate-to high …

We use deep Herschel observations taken with both PACS and SPIRE imaging cameras to
estimate the dust mass of a sample of galaxies extracted from the GOODS-S, GOODS-N and …

We describe JWST/NIRSpec prism measurements of Ly α emission in z≳ 5 galaxies. We
identify Ly α detections in 10 out of 69 galaxies with robust rest-optical emission-line redshift …

We investigate Lyα,[O iii] λ5007, Hα, and [C ii] 158 μm emission from 1124 galaxies at z= 4.9–
7.0. Our sample is composed of 1092 Lyα emitters (LAEs) at z= 4.9, 5.7, 6.6, and 7.0 …

Using wide-field narrow-band surveys, we provide a new measurement of the z= 6.6
Lymanα emitter (LAE) luminosity function (LF), which constraints the bright end for the first …