Results 11 to 20 of about 8,368 (167)
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 ...
Matthew Hayes
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Clustering of Lyman-Alpha Emitters galaxies
Abstract Galaxy clustering properties have been studied for decades to constrain cosmological parameters and have today, with large datasets of high-redshift sources piling up, become a powerful tool to discriminate and characterize primeval galaxies.
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Damped Lyman-alpha systems and galaxy formation
plain tex, 3 figures avalaible on ...
Mo, H. J., Miralda-Escude, J.
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We present the first publicly released catalog of sources obtained from the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX). HETDEX is an integral field spectroscopic survey designed to measure the Hubble expansion parameter and angular diameter ...
Erin Mentuch Cooper +45 more
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Keck Spectroscopy of Faint 3
As Lyman-alpha photons are scattered by neutral hydrogen, a change with redshift in the Lyman-alpha equivalent width distribution of distant galaxies offers a promising probe of the degree of ionization in the intergalactic medium and hence when cosmic ...
Ellis, Richard S. +2 more
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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
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
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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
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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
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

