Corrigendum

Corrigendum to “Clusters of Galaxies in a Weyl Geometric Approach to Gravity”

Figure 6

Comparison of dark/transparent/phantom mass halos for Coma in NFW, WST, and TeVeS models and free parameters of halos for NFW and TeVeS ( with neutrino core) adapted to mass data (black error bars) at and  kpc. Red error bar at expresses variability of the NFW halo at this distance due to adapting it to the given error interval of mass data at .