Oral title: AGN feedback does not destroy cold molecular gas in local luminous Seyfert galaxies

Oral abstract: I will report on a controlled study of CO in a complete sample of the most luminous nearby Seyfert galaxies 
from the LLAMA survey, the most advanced to date. Using constraints on gas fractions and star-formation efficiencies 
over the inner kpc, we test for the influence of the AGN on the very raw material of star-formation. We find no difference 
between AGN and inactive galaxies; the star-formation efficiencies in the centres of Seyferts are consistent with their 
larger-scale discs. Our results highlight the resilience of star-forming molecular gas to the effects of AGN feedback.