Results 91 to 100 of about 5,863 (203)

LATIS Data Release: ∼4200 Spectra of z ∼ 2–3 Galaxies, Redshifts, and Intergalactic Medium Tomography Maps

open access: yesThe Astrophysical Journal Supplement Series
We present the data release of the Ly α Tomography IMACS Survey (LATIS), one of the largest optical spectroscopic surveys of faint high-redshift galaxies.
Andrew B. Newman   +10 more
doaj   +1 more source

Lyman Alpha and MgII as Probes of Galaxies and their Environments

open access: yes, 2014
Lyα emission, Lyα absorption and MgII absorption are powerful tracers of neutral hydrogen. Hydrogen is the most abundant element in the universe and plays a central role in galaxy formation via gas accretion and outflows, as well as being the precursor to molecular clouds, the sites of star formation.
Barnes, Luke A.   +2 more
openaire   +2 more sources

Extreme damped Lyman-$\alpha$ absorption in young star-forming galaxies at $z=9-11$

open access: yes, 2023
The onset of galaxy formation is thought to be initiated by the infall of neutral, pristine gas onto the first protogalactic halos. However, direct constraints on the abundance of neutral atomic hydrogen (HI) in galaxies have been difficult to obtain at ...
Strait, Victoria B.   +20 more
core  

The galaxy-IGM connection in THESAN: the physics connecting the IGM Lyman-$α$ opacity and galaxy density in the reionization epoch

open access: yesThe Open Journal of Astrophysics
The relation between the Lyman-$\alpha$ effective optical depth of quasar sightlines ($\tau_\mathrm{los}$) and the distribution of galaxies around them is an emerging probe of the connection between the first collapsed structures and the IGM properties ...
Enrico Garaldi   +3 more
doaj   +1 more source

Metallicity Evolution of Damped Lyman-Alpha Galaxies

open access: yes, 2002
We have reanalyzed the existing data on Zinc abundances in damped Ly-alpha (DLA) absorbers to investigate whether their mean metallicity evolves with time. Most models of cosmic chemical evolution predict that the mass- weighted mean interstellar metallicity of galaxies should rise with time from a low value ~ 1/30 solar at z ~ 3 to a nearly solar ...
Kulkarni, Varsha P., Fall, S. Michael
openaire   +2 more sources

Lyman-Alpha Escape from Low-Mass, Compact, High-Redshift Galaxies

open access: yes, 2022
We investigate the effects of stellar populations and sizes on Ly$\alpha$ escape in 27 spectroscopically confirmed and 35 photometric Lyman-Alpha Emitters (LAEs) at z $\approx$ 2.65 in seven fields of the Bo\"otes region of the NOAO Deep Wide-Field ...
Dey, Arjun   +15 more
core   +1 more source

A Nitrogen-rich AGN Powering a Large Ionizing Bubble at z = 8.63

open access: yesThe Astrophysical Journal
We report the detection of Ly α in CANUCS-LRD-z8.6, a recently discovered active galactic nucleus (AGN) at z = 8.63 by R. Tripodi et al. ( 2025 ), in new NIRSpec/MSA G140H/F070LP observations.
Takahiro Morishita   +7 more
doaj   +1 more source

Lyman Break Galaxies and the Lyman-alpha Forest

open access: yes, 2002
We use hydrodynamic simulations to predict correlations between Lya forest absorption and galaxies at redshift z~3. The probability distribution function (PDF) of Lya flux decrements shifts systematically towards higher values in the vicinity of galaxies, reflecting the overdense environments in which these galaxies reside. The predicted signal remains
Kollmeier, Juna A.   +3 more
openaire   +2 more sources

Escape Fractions from Unattenuated Lyα Emitters around Luminous z > 6 Quasars

open access: yesThe Astrophysical Journal Letters
Ionized proximity zones around luminous quasars provide a unique laboratory to characterize the Ly α emission lines from z  > 6 galaxies without significant attenuation from the intergalactic medium (IGM).
Minghao Yue   +9 more
doaj   +1 more source

Lyman alpha emission in high-redshift galaxies

open access: yes, 2007
A significant fraction of the high-redshift galaxies show strong Lyman emission lines. For redshifts z>5, most known galaxies belong to this class. However, so far not much is known about the physical structure and nature of these objects. Our aim is to analyse the Lyman alpha emission in a sample of high-redshift UV-continuum selected galaxies and ...
Tapken, C.   +6 more
openaire   +2 more sources

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