Results 91 to 100 of about 182 (139)

Observing Lyman alpha emitters - How does Lyman alpha escape from galaxies?

open access: yes, 2016
The Lyman alpha (Lyα) emission line has grown to become one of the most successful tools for finding galaxies at high redshift. At redshifts corresponding to the early cosmic times of reionization and primeval galaxy formation, the wavelength of Lyα is still accessible with ground-based facilities.
openaire   +1 more source

ODIN: High Clustering Strength of Protoclusters at Cosmic Noon

open access: yesThe Astrophysical Journal
The One-hundred-deg ^2 DECam Imaging in Narrowbands (ODIN) survey is carrying out a systematic search for protoclusters during Cosmic Noon, using Ly α -emitting galaxies (LAEs) as tracers.
Vandana Ramakrishnan   +19 more
doaj   +1 more source

Cold and stable antimatter for fundamental physics. [PDF]

open access: yesProc Jpn Acad Ser B Phys Biol Sci, 2020
Yamazaki Y.
europepmc   +1 more source

High-resolution Observations of CO(3–2) in Haro 2: Cool Molecular Outflows of a Lyα Emitter

open access: yesThe Astronomical Journal
Haro 2 is a blue compact dwarf galaxy and the closest (at 21 Mpc) known Lyα emitter. UV and optical observations have found Haro 2 to be immersed in shells of partly ionized gas expanding at ∼200 km s ^−1 .
Sara Beck, Pei-Ying Hsieh, Jean Turner
doaj   +1 more source

Comparing Galaxies and Lyman Alpha Absorbers at Low Redshift

open access: yes, 1997
17 pages, 8 figures, accepted to the Astrophysical ...
openaire   +2 more sources

Subaru studies of the cosmic dawn. [PDF]

open access: yesProc Jpn Acad Ser B Phys Biol Sci, 2011
Iye M.
europepmc   +1 more source

Cosmology and fundamental physics with the Euclid satellite. [PDF]

open access: yesLiving Rev Relativ, 2018
Amendola L   +71 more
europepmc   +1 more source

Home - About - Disclaimer - Privacy