HIGHLIGHTS
- who: Debackere Stijn N. B. and colleagues from the University, , RA, The Netherlands have published the paper: Why are we still using 3D masses for cluster cosmology?, in the Journal: (JOURNAL)
- what: The main focus of these surveys is on measuring the matter distribution through the clustering of galaxies and through the lensing-induced distortion of galaxy shapes due to the intervening large-scale structure, the cosmic shear. The authors focus on weak lensing observations because they probe the total matter content and are thus less sensitive to uncertainties in how baryonic matter traces the . . .
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