Using angular pair upweighting to improve 3D clustering measurements

INIS

• galaxies 100%
• surveys 66%
• data 33%
• information 33%
• applications 33%
• spectra 33%
• reduction 33%
• red shift 33%
• correlation functions 33%
• oscillations 33%
• baryons 33%
• populations 33%
• barium oxides 33%
• monopoles 33%

Physics

• Surveys 66%
• Galaxies 66%
• Galaxy Clusters 33%
• Baryon 33%
• Oscillation 33%
• Information 33%
• Utilization 33%
• Model 33%
• Area 33%
• Targets 33%
• Populations 33%
• Optical Spectrum 33%
• Correlation 33%