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THE ERA OF STAR FORMATION IN GALAXY CLUSTERS
Published 2015“…We analyze the star formation properties of 16 infrared-selected, spectroscopically confirmed galaxy clusters at 1 < z < 1.5 from the Spitzer/IRAC Shallow Cluster Survey (ISCS). …”
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Characterising galaxy clusters’ completeness function in Planck
Published 2024-01-01“…Galaxy cluster number counts are an important probe to constrain cosmological parameters. …”
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Cosmology with galaxy clusters: An improved multiwavelength analysis
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Triplets of quasars as lighthouses of rich galaxy clusters
Published 2008“…In two out of three cases, the members of the triplets have been found on the periphery of an extremelly rich galaxy cluster (Abell class 2 and 3). The third triplet also appears associated with a very rich cluster of galaxies but on a somewhat larger scale. …”
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Weak-lensing Mass Bias in Merging Galaxy Clusters
Published 2023-01-01Subjects: “…Galaxy clusters…”
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New Metrics to Probe the Dynamical State of Galaxy Clusters
Published 2023-01-01“…We present new diagnostic metrics to probe the dynamical state of galaxy clusters. These novel metrics rely on the computation of the power spectra of the matter and gas distributions and their cross-correlation derived from cluster observations. …”
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Detection of Strongly Lensed Arcs in Galaxy Clusters with Transformers
Published 2022-01-01“…Strong lensing in galaxy clusters probes properties of dense cores of dark matter halos in mass, studies the distant universe at flux levels and spatial resolutions otherwise unavailable, and constrains cosmological models independently. …”
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Testing Screening Mechanisms with Mass Profiles of Galaxy Clusters
Published 2022-03-01Subjects: Get full text
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The nature of the motions of multiphase filaments in the centers of galaxy clusters
Published 2023-05-01Subjects: “…galaxy clusters…”
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Distribution of Hα Emitters in Merging Galaxy Clusters
Published 2024-01-01Subjects: “…Galaxy clusters…”
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Baryon content of massive galaxy clusters at 0.57
Published 2021“…We study the stellar, brightest cluster galaxy (BCG) and intracluster medium (ICM) masses of 14 South Pole Telescope (SPT) selected galaxy clusters with median redshift z = 0.9 and mass M500 = 6 × 1014M⊙. …”
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The impact of galaxy selection on the splashback boundaries of galaxy clusters
Published 2022“…<jats:title>Abstract</jats:title> <jats:p>We explore how the splashback radius (Rsp) of galaxy clusters, measured using the number density of the subhalo population, changes based on various selection criteria using the IllustrisTNG cosmological galaxy formation simulation. …”
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The impact of galaxy selection on the splashback boundaries of galaxy clusters
Published 2022“…<jats:title>Abstract</jats:title> <jats:p>We explore how the splashback radius (Rsp) of galaxy clusters, measured using the number density of the subhalo population, changes based on various selection criteria using the IllustrisTNG cosmological galaxy formation simulation. …”
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Evolution of Supermassive Black Hole Feedback in Galaxy Clusters
Published 2024“…Galaxy clusters, the largest gravitationally-bound structures in the Universe, are superb laboratories for studying the baryon cycle that governs the evolution of all galaxies. …”
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