The mass structure of the galaxy cluster Cl0024+1654 from a full lensing analysis of joint subaru and ACS/NIC3 observations

Keyphrases

• Lensing 100%
• Galaxy Clusters 100%
• Mass Profiles 100%
• Subaru 100%
• Virion 66%
• Mass Distribution 66%
• Model-independent 66%
• Weak Lensing 66%
• Strong Lensing 66%
• Galaxies 33%
• Line-of-sight 33%
• X-ray 33%
• Well-defined 33%
• Light Profile 33%
• Whole Systems 33%
• Data-centric 33%
• High-resolution 33%
• Virial Mass 33%
• Hubble Space Telescope 33%
• Model Fitting 33%
• Cluster Mass 33%
• Declining Trend 33%
• Data Overlap 33%
• White Model 33%
• Color Information 33%
• Pre-merger 33%
• Gravitational Potential 33%
• Accurate Mass 33%
• Post-collision 33%
• Unbound Materials 33%
• Positional Information 33%
• Collision Simulation 33%
• Cluster System 33%
• Cluster Collisions 33%

Physics

• Galaxy Clusters 100%
• Mass Distribution 100%
• Line of Sight 50%
• Hubble Space Telescope 50%
• High Resolution 50%
• Gravitational Field 50%