Results 21 to 30 of about 572 (187)
Clustering of galaxies at high redshifts [PDF]
Monthly Notices of the Royal Astronomical Society, 1998 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.
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Methods for identifying high‐redshift galaxy cluster candidates [PDF]
Astronomische Nachrichten, 2019 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
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The Association of Galaxy Clusters with Moderately-High-Redshift Quasars [PDF]
Symposium - International Astronomical Union, 1986 CCD images of quasars having redshifts between 0.3 and 0.65 are analyzed to study the association of galaxies with quasars. Average luminosity functions (LF) of the excess galaxies associated with the radio-loud quasars are determined. It is found that for the sub-sample with z>0.55, there is a significant brightening of the characteristic magnitude
H. K. C. Yee, Richard F. Green
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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
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The observed properties of high-redshift cluster galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 1995 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
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Implications of multiple high-redshift galaxy clusters [PDF]
Physical Review D, 2011 11 pages, 7 figures, modified to match published ...
Ben Hoyle, Raul Jimenez, Licia Verde
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Optical signatures of high-redshift galaxy clusters [PDF]
The Astrophysical Journal, 1994 We combine an N-body and gasdynamic simulation of structure formation with an updated population synthesis code to explore the expected optical characteristics of a high-redshift cluster of galaxies. We examine a poor (2 keV) cluster formed in a biased, cold dark matter cosmology and employ simple, but plausible, threshold criteria to convert gas into ...
Evrard, August E., Charlot, S.
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The clustering properties of high-redshift passive galaxies
Monthly Notices of the Royal Astronomical Society: Letters, 2023 ABSTRACT We investigate the clustering properties of 3 < z < 5 candidate passive galaxies from the Merlin et al. (2019) sample residing in the GOODS-North (35 sources) and GOODS-South (33 sources) fields. Within the large uncertainties due to the paucity of sources we do not detect clustering signal in GOODS-North, while ...
M Magliocchetti +3 more
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Hawaii Two-0: high-redshift galaxy clustering and bias [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT We perform an analysis of two-point galaxy clustering and galaxy bias using Subaru Hyper-Suprime Cam (HSC) data taken jointly by the Subaru Strategic Program and the University of Hawaii in the Cosmic Evolution Survey (COSMOS) field over an area of 1.8 sq deg.
Róbert Beck +4 more
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Tracing the Total Stellar Mass and Star Formation of High-redshift Protoclusters
The Astrophysical Journal, 2023 As the progenitors of present-day galaxy clusters, protoclusters are excellent laboratories to study galaxy evolution. Since existing observations of protoclusters are limited to the detected constituent galaxies at UV and/or infrared wavelengths, the ...
Roxana Popescu +8 more
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