Results 91 to 100 of about 182 (139)
Observing Lyman alpha emitters - How does Lyman alpha escape from galaxies?
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
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]
Yamazaki Y.
europepmc +1 more source
High-resolution Observations of CO(3–2) in Haro 2: Cool Molecular Outflows of a Lyα Emitter
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
17 pages, 8 figures, accepted to the Astrophysical ...
openaire +2 more sources
Gamma-ray bursts and their use as cosmic probes. [PDF]
Schady P.
europepmc +1 more source
Subaru studies of the cosmic dawn. [PDF]
Iye M.
europepmc +1 more source
Cosmology and fundamental physics with the Euclid satellite. [PDF]
Amendola L +71 more
europepmc +1 more source
The universe at z > 5: when and how did the "dark age" end? [PDF]
Rees MJ.
europepmc +1 more source
Global preventive feedback of powerful radio jets on galaxy formation. [PDF]
Cen R.
europepmc +1 more source

