Results 141 to 150 of about 5,863 (203)
Context. Wide-field narrowband surveys are an efficient way of searching large volumes of high-redshift space for distant galaxies. Aims. We describe the Wide Field Imager Lyman-Alpha Search (WFILAS) over 0.74 sq.
Athreya, Ramana M +8 more
core +1 more source
CLASSY. XI. Tracing Neutral Gas Properties Using UV Absorption Lines and 21 cm Observations
Rest-frame far-ultraviolet (FUV) observations from JWST are revolutionizing our understanding of the high- z galaxies that drove reionization and the mechanisms by which they accomplished it.
Kaelee S. Parker +17 more
doaj +1 more source
Lyman alpha radiation in external galaxies
The Ly alpha line of atomic hydrogen is often a luminous component of the radiation emitted by distant galaxies. Except for those galaxies which have a substantial central source of non-stellar ionizing radiation, most of the Ly alpha radiation emitted ...
Mckee, Christopher F., Neufeld, David A.
core
Verifying the mass-metallicity relation in damped Lyman-alpha selected galaxies at 0.1<z<3.2
A scaling relation has recently been suggested to combine the galaxy mass-metallicity (MZ) relation with metallicities of damped Lyman-alpha systems (DLAs) in quasar spectra.
Zafar, T. +3 more
core +1 more source
The Lyα and Continuum Origins Survey. I. Survey Description and Lyα Imaging
Understanding the mechanisms driving the escape of ionizing or Lyman continuum (LyC) emission from the interstellar medium of galaxies is necessary to constrain the evolution of reionization and the sources responsible for it.
Alexandra Le Reste +27 more
doaj +1 more source
The Lyman alpha (Lyα) emission line from the recombination of hydrogen atoms is predicted to be the strongest spectral feature of galaxies. This emission line is regularly used to detect and characterise high redshift galaxies.
Bacon, Roland, +2 more
core
On the Physical Nature of Lyα Transmission Spikes in High-redshift Quasar Spectra
We investigate Lyman-alpha (Ly α ) transmission spikes at 5.2 < z < 6.8 using synthetic quasar spectra from the “Cosmic Reionization on Computers” simulations.
Hanjue Zhu +2 more
doaj +1 more source
Galaxies are surrounded by a copious amont of extended gas, mostly composed of neutral hydrogen. This area, called the circumgalactic medium (CGM), is the place of gas exchanges between the host galaxy and its close environnement, and so the CGM is a ...
Claeyssens, Adélaïde
core
We present luminosity functions (LFs) and angular correlation functions (ACFs) derived from 18,960 Ly α emitters (LAEs) at z = 2.2−7.3 over a wide survey area of ≲24 deg ^2 that are identified in the narrowband data of the HSC-SSP and CHORUS surveys ...
Hiroya Umeda +13 more
doaj +1 more source
Design For The First Narrowband Filter For The Dark Energy Camera: Optimizing The LAGER Survey For Z ~ 7 Galaxies. [PDF]
Zheng ZY +24 more
europepmc +1 more source

