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Structure of the Coma Cluster of Galaxies

https://doi.org/10.1086/110933
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A SPECTROSCOPICALLY CONFIRMED EXCESS OF 24 μm SOURCES IN A SUPER GALAXY GROUP ATz= 0.37: ENHANCED DUSTY STAR FORMATION RELATIVE TO THE CLUSTER AND FIELD ENVIRONMENT
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SG1120-1202: Mass-quenching as Tracked by UV Emission in the Group Environment at z = 0.37
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Lyα Absorbers and the Coma Cluster
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Galaxy Merger Fractions in Two Clusters at Using the Hubble Space Telescope
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Physical Properties of a Coma-analog Protocluster at z = 6.5
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MOSEL: Strong [Oiii] 5007 Å Emitting Galaxies at (3 < z < 4) from the ZFOURGE Survey
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Selection of Massive Evolved Galaxies at 3 ≤ z ≤ 4.5 in the CANDELS Fields
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Spectroscopic Confirmation of Two Extremely Massive Protoclusters, BOSS1244 and BOSS1542, at z = 2.24
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An Alternative to Dark Matter? Part 3: An Open Universe (3 Gy to 76 Gy) Galaxies and Structures Rotation
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The mass distribution in an assembling super galaxy group at $z=0.37$
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Convergence and scatter of cluster density profiles
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THE NEW HORIZON RUN COSMOLOGICAL N-BODY SIMULATIONS
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NUMERICAL SIMULATIONS OF GALAXY FORMATION
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Exploring The Foundations and Applications of Cosmological Simulation
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Preparation for the analysis and interpretation of Euclid galaxy clusters
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Numerical methods for the prediction of gravitational lensing signal as a probe of the mass content on the Universe
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