The mm-to-cm SED of spiral galaxies. Synergies between NIKA2 and SRT
  instruments
  The mm-to-cm range of the Spectral Energy Distribution of spiral galaxies
remains largely unexplored. Its coverage is required to disentangle the
contribution of dust emission, free-free and synchrotron radiation and can
provide constraints on dust models, star-formation rates and ISM properties. We
present the case for a synergy between NIKA2 observations of nearby spirals and
those from planned and current instrumentation at the Sardinia Radio Telescope,
and report on a pilot K-band program to search for Anomalous Microwave
Emission, an elusive emission component which is presumably related to dust.
