  That active galactic nuclei (AGN) with jets can alternately enhance as well
as suppress star formation rates, explains the location and slope of radio loud
AGN on the star formation rate-stellar mass plane. Here, we explore 860 type 1
and 2 AGN at z<0.2 from the ROSAT-2XRS survey in order to understand both
different location and lower slopes for non-jetted AGN in the star formation
rate-stellar mass plane. We describe the nature of these differences in terms
of different degrees of black hole feedback, with relatively weak negative
feedback from non-jetted AGN compared to both relatively strong positive and
negative feedback from jetted AGN. The validity of these ideas brings us a step
closer towards understanding the black hole scaling relation across space and
time.

Astrophysics of Galaxies