Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations

Keyphrases

• Autocorrelation 50%
• CDM Model 50%
• Cluster Density 50%
• Cosmological Constraints 100%
• Cosmological Parameters 50%
• Cosmology 50%
• Dark Energy Survey 100%
• First Year 50%
• Galaxies 100%
• Galaxy Clusters 50%
• Imaging Surveys 50%
• Joint Analysis 100%
• Mass Scaling 50%
• Multi-probe 50%
• Scaling Relations 50%
• Two-point Correlation 50%
• Two-point Correlation Function 50%
• Weak Gravitational Lensing 50%
• Weak Lensing 100%
• Weak-galaxies 100%

Physics

• Cosmological Parameters 50%
• Cross Correlation 100%
• Field Galaxies 50%
• Galaxy Clusters 50%
• Gravitational Lensing Shear 50%
• Weak Gravitational Lensing 50%