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Scaling Properties of Galaxy Groups
Published 2021-05-01Subjects: “…galaxy groups…”
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The Metal Content of the Hot Atmospheres of Galaxy Groups
Published 2021-06-01“…Galaxy groups host the majority of matter and more than half of all the galaxies in the Universe. …”
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Constraints on the Optical Depth of Galaxy Groups and Clusters
Published 2017“…This signal probes the matter-velocity correlation function, scaled by the average optical depth (τ) of the galaxy groups and clusters in the sample, and is thus of fundamental importance for cosmology. …”
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Search for Dark Matter Annihilation in Galaxy Groups
Published 2018“…We use 413 weeks of publicly available Fermi Pass 8 gamma-ray data combined with recently developed galaxy group catalogs to search for evidence of dark matter annihilation in extragalactic halos. …”
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Kinematic unrest of low mass galaxy groups
Published 2020“…In an effort to better understand the formation of galaxy groups, we examine the kinematics of a large sample of spectroscopically confirmed X-ray galaxy groups in the Cosmic Evolution Survey (COSMOS) with a high sampling of galaxy group members up to $z=1$. …”
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The cosmological constant derived via galaxy groups and clusters
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Feedback from Active Galactic Nuclei in Galaxy Groups
Published 2021-05-01Subjects: Get full text
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Somewhere in between: Tracing the Radio Emission from Galaxy Groups (or Why Does the Future of Observing Galaxy Groups with Radio Telescopes Look Promising?)
Published 2021-10-01Subjects: “…galaxy groups…”
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Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galaxies
Published 2020“…We present a study of 107 galaxies, groups, and clusters spanning ∼3 orders of magnitude in mass, ∼5 orders of magnitude in central galaxy star formation rate (SFR), ∼4 orders of magnitude in the classical cooling rate () of the intracluster medium (ICM), and ∼5 orders of magnitude in the central black hole accretion rate. …”
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REVISED MASS-TO-LIGHT RATIOS FOR NEARBY GALAXY GROUPS AND CLUSTERS
Published 2015“…For the mass range covered by our sample, the assumption of a Chabrier initial mass function (IMF) yields an integrated M*/L[subscript i] [~ over bar] 1.7 ± 0.2 M [subscript ☉]/L[subscript i], [subscript ☉], a lower value than used in most similar studies, though consistent with the study of low-mass galaxy groups by Leauthaud et al. A light (diet) Salpeter IMF would imply a ~60% increase in M*/L[subscript i].…”
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WALLABY early science – I. The NGC 7162 galaxy group
Published 2018“…We present Widefield ASKAP L-band Legacy All-sky Blind Survey (WALLABY) early science results from the Australian Square Kilometre Array Pathfinder (ASKAP) observations of the NGC 7162 galaxy group. We use archival HIPASS and Australia Telescope Compact Array (ATCA) observations of this group to validate the new ASKAP data and the data reduction pipeline ASKAP SOFT. …”
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The 2dF galaxy redshift survey: The clustering of galaxy groups
Published 2004“…We measure the clustering of galaxy groups in the 2dFGRS Percolation-Inferred Galaxy Group (2PIGG) catalogue. …”
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A Fast Radio Burst in a Compact Galaxy Group at z ∼ 1
Published 2024-01-01Subjects: Get full text
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Galaxy Quenching with Mass Growth History of Galaxy Groups and Clusters: The Importance of Post-processing
Published 2023-01-01Subjects: Get full text
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Statistical Association between the Candidate Repeating FRB 20200320A and a Galaxy Group
Published 2024-01-01“…We demonstrate that the correlation arises surprisingly because of a statistical association between FRB 20200320A (extragalactic DM ≈ 550 pc cm ^−3 ) and a galaxy group in the same dark matter halo at redshift z ≈ 0.32. …”
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