Results 31 to 40 of about 5,863 (203)
We use large simulations of Ly α emitters with different fractions of ionized intergalactic medium to quantify the clustering of Ly α emitters as measured by the void probability function (VPF), and how it evolves under different ionization scenarios. We
Lucia A. Perez +3 more
doaj +1 more source
Early Results from GLASS-JWST. XXIII. The Transmission of Lyα from UV-faint z ∼ 3–6 Galaxies
Ly α emission from galaxies can be used to trace neutral hydrogen in the epoch of reionization, however, there is a degeneracy between the attenuation of Ly α in the intergalactic medium (IGM) and the line profile emitted by the galaxy.
Gonzalo Prieto-Lyon +20 more
doaj +1 more source
On the Diffuse Lyman-alpha Halo Around Lyman-alpha Emitting Galaxies
11 pages, 8 figures, accepted for publication in ApJ. Our conclusion is slightly updated as a result of an improved evaluation of the sky-subtraction systematics in the observed UV profile.
Lake, Ethan +5 more
openaire +2 more sources
The HETDEX Survey Emission-line Exploration and Source Classification
The Hobby–Eberly Telescope Dark Energy Experiment (HETDEX) is an untargeted spectroscopic survey that aims to measure the expansion rate of the universe at z ∼ 2.4 to 1% precision for both H ( z ) and D _A ( z ).
Dustin Davis +22 more
doaj +1 more source
Lyman-alpha emission in star-forming galaxies
IUE observations of five blue, low-metallicity, star-forming galaxies sufficiently redshifted to permit detection of Lyman-alpha are reported. The galaxies with metallicities 0.1 time solar or more have weak or absent Lyman-alpha emission. There is evidence for increasing Lyman-alpha emission with decreasing metallicity.
Lee W. Hartmann +4 more
openaire +1 more source
Transfert radiatif Lyman-alpha dans les galaxies
Pour étudier la formation et l'évolution des Galaxies, nous avons développé un code de transfert radiatif des photons Lyman-alpha à travers le milieu interstellaire d'une galaxie, MCLya. Emise par les atomes d'hydrogènes excités, cette raie de résonnance
Verhamme, Anne
core +1 more source
Lyman-continuum galaxies and the escape fraction of Lyman-break galaxies
Lyman-break galaxies (LBGs) at z ̃ 3-4 are targeted to measure the fraction of Lyman-continuum (LyC) flux that escapes from high-redshift galaxies. However, z ̃ 3-4 LBGs are identified using the Lyman-break technique which preferentially selects galaxies
C. Gonzalo Diaz (19100915) +3 more
core +1 more source
We present Ly α imaging of 45 low-redshift star-forming galaxies observed with the Hubble Space Telescope. The galaxies have been selected to have moderate to high star formation rates (SFRs) using far-ultraviolet (FUV) luminosity and H α equivalent ...
Jens Melinder +20 more
doaj +1 more source
ABSTRACT The goal of this study is to confirm the feasibility of the use of digitized low dispersive MtWilson Michigan Southern Sky Hα$$ \alpha $$ survey astronomical photographic plates for modern astrophysical research. The detection of highly redshifted objects, such as early galaxies and quasars, is fundamental to understanding the universe's ...
Tauseef Ahmad Zafar +3 more
wiley +1 more source
The relationship between Gas and Galaxies [PDF]
We have investigated the 2D 2-point correlation function, ƐAG, between low column density Lya absorbers and galaxies at a redshift z ~ 1 for the first time.
Shone, Allen Maurice
core

