The SRG/eROSITA All-Sky Survey $J$-Band Follow-Up Observations for Selected High-Redshift Galaxy Cluster Candidates [PDF]
N. Zimmermann +23 more
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First simultaneous optical/near-infrared imaging of an X-ray selected, high-redshift cluster of galaxies with GROND [PDF]
D. Pierini +30 more
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Clusters of galaxies host spectacular diffuse radio sources, extending over scales from 100 kpc to several Mpcs. These sources, with extremely faint surface brightness ( μ Jy/arcsec ^2 level), are not tied to individual galaxies but trace synchrotron ...
Julie HLavacek-Larrondo +12 more
doaj +1 more source
The galaxy cluster RXJ 0152.7-1357 is emitting X-rays at the high rate of 148 counts $ks^{-1}$. It would be one of the most luminous X-ray clusters known if it is at its redshift distance of z = .8325.
Arp, H.
core +1 more source
Ram‐Pressure Stripping of Galaxies in High‐Redshift Clusters and the Influence of Intracluster Medium Heating [PDF]
Yutaka Fujita
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Cluster Candidates with Massive Quiescent Galaxies at z ∼ 2
Galaxy clusters are crucial to understanding the role of the environment in galaxy evolution. However, due to their rarity, only a limited number of clusters have been identified at z ≳ 2. In this paper, we report a discovery of seven cluster candidates
Tomokazu Kiyota +9 more
doaj +1 more source
Constraining ${Ω_{0}}$ from X-ray properties of Clusters of Galaxies at high redshift [PDF]
R. Sadat, Alain Blanchard, J. Oukbir
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The Photometric Analysis of the Environment Around Two Dusty Star-forming Galaxies at z ∼ 2
Studying the environments of dusty star-forming galaxies (DSFGs) provides insight into whether these luminous systems are reliable signposts of large-scale overdensities.
Joe Bhangal +9 more
doaj +1 more source
LAE Galaxies at High Redshift: Formation Sites for Low-Metal Globular Clusters [PDF]
Bruce G. Elmegreen +2 more
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Identification of Galaxy Protoclusters Based on the Spherical Top-hat Collapse Theory
We propose a new method for finding galaxy protoclusters that is motivated by structure formation theory and also directly applicable to observations. We adopt the conventional definition that a protocluster is a galaxy group whose virial mass M _vir < M
Jaehyun Lee +9 more
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