Context. This paper presents a study of the galaxy Lyman-alpha luminosity function (LF)
using a large sample of 17 lensing clusters observed by the Multi Unit Spectroscopic …

We study the ionizing photon production efficiency at the end of the Epoch of Reionization
(z∼ 5.4− 6.6) for a sample of 30 Ly α emitters. This is a crucial quantity to infer the ionizing …

The Lyman alpha emission line (Lyα) of neutral hydrogen (Hi) is intrinsically the brightest
emission feature in the spectrum of astrophysical nebulae, making it a very attractive …

Abstract Far-ultraviolet (FUV;∼ 1200–2000 Å) spectra are fundamental to our understanding
of star-forming galaxies, providing a unique window on massive stellar populations …

The Keck Lyman Continuum Spectroscopic Survey (KLCS): The Emergent Ionizing Spectrum
of Galaxies at z ∼ 3 - IOPscience This site uses cookies. By continuing to use this site you …

We report the detection of extended Lyα haloes around 145 individual star-forming galaxies
at redshifts 3≤ z≤ 6 in the Hubble Ultra Deep Field observed with the Multi-Unit …

We report the detection of extended Lyα emission around individual star-forming galaxies at
redshifts z= 3− 6 in an ultradeep exposure of the Hubble Deep Field South obtained with …

ABSTRACT We report Hubble Space Telescope/Cosmic Origins Spectrograph observations
of the Lyα emission and interstellar absorption lines in a sample of 10 star-forming galaxies …

At redshift z> 5, the far-infrared (FIR) continuum spectra of main-sequence galaxies are
sparsely sampled, often with a single data point. The dust temperature T d, SED, thus has to …

We infer the properties of massive star populations using the far-ultraviolet stellar continua of
61 star-forming galaxies: 42 at low redshift observed with the Hubble Space Telescope and …