Galaxy cluster mass density profile derived using the submillimetre galaxies magnification bias

In this work we want to study the average mass density profile of tens to hundreds of clusters of galaxies acting as lenses that produce a magnification bias on the SMGs, and to estimate their associated masses and concentrations for different richness ranges. The background sample is composed of SMGs observed by Herschel with 1.2

Keywords:

• Estimator
• Galaxy group
• Galaxy cluster
• Redshift
• Galactic halo
• Physics
• Astrophysics
• Cluster (physics)
• Galaxy
• Halo

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