The Clustering of High‐Redshift Galaxies in the Cold Dark Matter Scenario [PDF]
The Astrophysical Journal, 1999 33 pages, 10 figures, AAS LaTeX (aaspp4.sty), submitted to ...
Katz, N, Hernquist, L, Weinberg, DH
openaire +3 more sources
The Evolution of Galaxies in and around Clusters at High-Redshift [PDF]
Publications of the Astronomical Society of Japan, 2004 Abstract In this paper, we focus on ram-pressure stripping and evaporation of disk galaxies in and around a cluster. We show that the evolution of the disk surface density affects the efficiency of ram-pressure stripping of galaxies at $z\gtrsim 1$.
Fujita, Yutaka, Goto, Tomotsugu
openaire +2 more sources
THE RED-SEQUENCE LUMINOSITY FUNCTION IN MASSIVE INTERMEDIATE-REDSHIFT GALAXY CLUSTERS [PDF]
, 2008 We measure the rest-frame B-band luminosity function of red-sequence galaxies of five intermediate-redshift (0.5 < z < 0.9), high-mass (σ>950 km s−1) clusters. Cluster galaxies are identified through photometric redshifts based on imaging in seven bands (
Steven M. Crawford +2 more
semanticscholar +1 more source
Galaxy Clusters Selected via the Sunyaev–Zel'dovich Effect in the SPTpol 100-square-degree Survey [PDF]
, 2020 We present a catalog of galaxy cluster candidates detected in 100 square degrees surveyed with the SPTpol receiver on the South Pole Telescope. The catalog contains 89 candidates detected with a signal-to-noise ratio greater than 4.6.
Crites, A. T. +3 more
core
Clustering of galaxies in a hierarchical universe -- II. Evolution to high redshift [PDF]
Monthly Notices of the Royal Astronomical Society, 1999 21 pages, Latex, 11 figures included, submitted to MNRAS; figure 11 ...
Kauffmann G. +3 more
openaire +2 more sources
Near-Infrared Properties of Moderate-Redshift Galaxy Clusters: Luminosity Functions and Density Profiles [PDF]
, 2006 We present K-band imaging for 15 of the CNOC1 clusters. The extensive spectroscopic data set available for these clusters allows us to determine the cluster K-band luminosity function and density profile without the need for statistical background ...
A. Muzzin +6 more
semanticscholar +1 more source
Expectations For an Interferometric Sunyaev-Zel'dovich Effect Survey for Galaxy Clusters [PDF]
, 2000 Non-targeted surveys for galaxy clusters using the Sunyaev-Zel'dovich effect (SZE) will yield valuable information on both cosmology and evolution of the intra-cluster medium (ICM). The redshift distribution of detected clusters will constrain cosmology,
Barbosa D. +7 more
core +2 more sources
A unified model for the maximum mass scales of molecular clouds, stellar clusters and high-redshift clumps [PDF]
, 2017 We present a simple, self-consistent model to predict the maximum masses of giant molecular clouds (GMCs), stellar clusters and high-redshift clumps as a function of the galactic environment.
M. Reina-Campos, J. Kruijssen
semanticscholar +1 more source
A Study of Nine High-Redshift Clusters of Galaxies. I. The Survey [PDF]
The Astronomical Journal, 1998 Accepted for publication in the Astronomical Journal.
Oke, J. B., Postman, Marc, Lubin, Lori
openaire +2 more sources
Ultra-low-frequency Gravitational Waves from Massive Clusters at z ∼ 1
The Astrophysical Journal, 2023 Recent progress with pulsar timing array experiments, especially from the NANOGrav collaboration, indicates that we are on the cusp of detecting significant signals from the inspiral of supermassive black hole (BH) binaries.
David K. Wendt, Roger W. Romani
doaj +1 more source