SAFIR: testing the coexistence of AGN and star formation activity and
  the nature of the dusty torus in the local universe
  We present the Seyfert and star formation Activity in the Far-InfraRed
(SAFIR) project, a small (15.1h) Herschel guaranteed time proposal performing
PACS and SPIRE imaging of a small sample of nearby Seyfert galaxies. This
project is aimed at studying the physical nature of the nuclear IR emission by
means of multi-component spectral energy distribution (SED) fitting and the
star formation properties of AGN hosts, as traced by cold dust. We summarize
the results achieved so far and outline the on-going work.
