A characterization of the diffuse Galactic emissions at large angular
  scales using the Tenerife data
  The Anomalous microwave emission (AME) has been proved to be an important
component of the Galactic diffuse emission in the range from 20 to 60 GHz. To
discriminate between different models of AME low frequency microwave data from
10 to 20 GHz are needed. We present here a re-analysis of published and
un-published Tenerife data from 10 to 33 GHz at large angular scales (from 5 to
15 degrees). We cross-correlate the Tenerife data to templates of the main
Galactic diffuse emissions: synchrotron, free-free and thermal dust. We find
evidence of dust correlated emission in the Tenerife data that could be
explained as spinning dust grain emission.
