Results 31 to 40 of about 8,408 (187)
The Lyman Alpha Reference Sample
Aims.We useHubbleSpace Telescope data of 45 nearby star-forming galaxies to investigate properties of Lyman-alpha (Lyα) halos, Lyαmorphology, and the star-forming characteristics of galaxies. We study how the morphology of Lyαemission is related to other Lyαobservables.
Rasekh, A. +9 more
openaire +3 more sources
HETDEX Public Source Catalog 1—Stacking 50,000 Lyman Alpha Emitters
We describe the ensemble properties of the 1.9 < z < 3.5 Lyman alpha emitters (LAEs) found in the HETDEX survey’s first public data release, HETDEX Public Source Catalog 1.
Dustin Davis +27 more
doaj +1 more source
Intensity Mapping of Lyman-alpha Emission During the Epoch of Reionization [PDF]
We calculate the absolute intensity and anisotropies of the Lyman-alpha radiation field present during the epoch of reionization. We consider emission from both galaxies and the intergalactic medium (IGM) and take into account the main contributions to ...
Asantha Cooray +58 more
core +3 more sources
The Relationship between IGM Lyα Opacity and Galaxy Density near the End of Reionization
Observed scatter in the Ly α opacity of quasar sightlines at z < 6 has motivated measurements of the correlation between Ly α opacity and galaxy density, as models that predict this scatter make strong and sometimes opposite predictions for how they ...
Holly M. Christenson +8 more
doaj +1 more source
To appear in "Gas and Galaxy Evolution", ASP Conference Series, eds. Hibbard, Rupen, and van Gorkum.
Turnshek, D. +6 more
openaire +2 more sources
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
Lyman Alpha Emitting Galaxies in the Nearby Universe [PDF]
AbstractThe 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 observational feature with which to survey galaxies. Moreover as an ultraviolet resonance line, Lyα possesses several unique characteristics that make it useful to ...
openaire +2 more sources
HOW LYMAN ALPHA EMISSION DEPENDS ON GALAXY STELLAR MASS [PDF]
ABSTRACT In this work, we show how the stellar mass (M *) of galaxies affects the 3 < z < 4.6 Lyα equivalent width (EW) distribution. To this end, we design a sample of 629 galaxies in the M * range from the ...
Grecco A. Oyarzún +8 more
openaire +3 more sources
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 Lyman-Alpha Emission of Starburst Galaxies [PDF]
7 PostScript pages with 4 Figures (included), astro-ph ...
openaire +2 more sources

