Results 21 to 30 of about 16,096,383 (218)
ODIN: Where Do Lyα Blobs Live? Contextualizing Blob Environments within Large-scale Structure
While many Ly α blobs (LABs) are found in and around several well-known protoclusters at high redshift, how they trace the underlying large-scale structure is still poorly understood. In this work, we utilize 5352 Ly α emitters (LAEs) and 129 LABs at z =
Vandana Ramakrishnan +18 more
doaj +1 more source
The clustering and host haloes of galaxy mergers at high redshift [PDF]
10 pages, 5 figures, accepted in MNRAS, version matches published ...
Wetzel, Andrew R. +2 more
openaire +2 more sources
Spatial clustering of high-redshift Lyman-break galaxies [PDF]
Accepted for publication in ...
Jose, Charles +3 more
openaire +2 more sources
Clustering of galaxies at high redshifts [PDF]
Recent observations show a large concentration of galaxies at high redshift. At first sight, strong clustering of galaxies at high redshifts seems to be in contradiction with the models of structure formation. In this paper we show that such structures are a manifestation of the strong clustering of rare peaks in the density field.
openaire +1 more source
Methods for identifying high‐redshift galaxy cluster candidates [PDF]
AbstractRecent theories linked long gamma ray bursts (GRBs) to galaxies with rapid star formation or starburst; thus, we expect that long GRBs (LGRBs) are more frequent in midcluster galaxies where mergers and tidal interactions between gas‐rich galaxies are more likely to occur. Yet there is no galaxy cluster known to be associated with LGRBs.
Pinter, Sandor +5 more
openaire +2 more sources
The Clustering of High‐Redshift Galaxies in the Cold Dark Matter Scenario [PDF]
33 pages, 10 figures, AAS LaTeX (aaspp4.sty), submitted to ...
Katz, N, Hernquist, L, Weinberg, DH
openaire +4 more sources
Accelerated Structural Evolution of Galaxies in a Starbursting Cluster at z = 2.51
Structural properties of cluster galaxies during their peak formation epoch, z ∼ 2–4 provide key information on whether and how the environment affects galaxy formation and evolution.
Can Xu +13 more
doaj +1 more source
The observed properties of high-redshift cluster galaxies [PDF]
We use the semi-analytic models of galaxy formation developed by Kauffmann, White \& Guiderdoni to generate predictions for the observed properties of cluster and group galaxies at redshifts between 0 and 0.6. We examine four sets of cosmological initial conditions: low-density CDM models with and without cosmological constant, a flat CDM model and
openaire +2 more sources
Implications of multiple high-redshift galaxy clusters [PDF]
11 pages, 7 figures, modified to match published ...
Ben Hoyle, Raul Jimenez, Licia Verde
openaire +3 more sources
A high redshift sample of x-ray selected galaxy clusters [PDF]
This thesis describes the creation of a X-ray selected galaxy cluster catalogue — the Southern Serendipitous High-redshift Archival ROSAT Cluster (SHARC) catalogue — and the use of the high-redshift subsample in constraining models of structure formation.
Burke, Douglas John
core +4 more sources

