The ALMA-ALPINE [CII] survey is aimed at characterizing the properties of a sample of
normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) …

The [C II] 158 μm line is one of the strongest IR emission lines, which has been shown to
trace the star formation rate (SFR) of galaxies in the nearby Universe, and up to z∼ 2 …

The cosmic ionizing emissivity from star-forming galaxies has long been anchored to UV
luminosity functions. Here, we introduce an emissivity framework based on Lyα emitters …

We measure, for the first time, the median equivalent width (EW) of Hα+[N ii] in star-forming
galaxies at z∼ 8. Our estimate leverages the unique photometric depth of the Spitzer/IRAC …

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 …

Recent work has shown that UV-luminous reionization-era galaxies often exhibit strong
Lyman-alpha emission despite being situated at redshifts where the IGM is thought to be …

The Atacama Large Millimeter Array (ALMA) Large Program to INvestigate [CII] at Early
times (ALPINE) targets the [CII] 158 μm line and the far-infrared continuum in 118 …

We investigate the degree of dust obscured star formation in 49 massive (log10 (M⋆/M⊙)>
9) Lyman-break galaxies (LBGs) at z= 6.5–8 observed as part of the Atacama Large …

We present the first results from the X-SHOOTER Lyman α survey at z= 2 (XLS-z 2). XLS-z 2
is a deep spectroscopic survey of 35 Lyman α emitters (LAEs) utilizing≈ 90 h of exposure …

The Ly α emission line is one of the most promising probes of cosmic reionization but
isolating the signature of a change in the ionization state of the intergalactic medium (IGM) is …