  In the current picture of cosmology and astrophysics, the formation and
evolution of galaxies is closely linked to that of their dark matter haloes.
The best representation of this galaxy-dark matter halo co-evolution is the M*
- Mhalo relation. In this study we investigate how the radio-mode feedback from
active galactic nuclei (AGN) affects the M* - Mhalo relation at redshifts 0.08
< z < 1.53. We use a set of 111 radio-selected AGN at 3 GHz VLA-COSMOS within
the X-ray galaxy groups in the COSMOS field. We compare these results to the
ones of 171 star-forming galaxies (SFGs), using the theoretical relation of
Moster et al. (2013). We find that AGN agree within 1% with the Moster et al.
(2013) relation, SFGs show an offset of 37%, suggesting that the radio-mode
feedback from AGN at a median redshift of ~ 0.5 still plays a significant role
in the M* - Mhalo relation.
