Setting the gold standard for the golden age of radio surveys

Extragalactic radio surveys are known to detect diverse objects - a mix of star-formation and accretion dominated sources. However, the details of that mixture have profound consequences for our understanding of the relationship between star-formation and accretion over cosmic history, and 'addressing this properly' within a probabilistic framework has until recently been impossible because (i) the necessary data did not exist, and (ii) it was too computationally expensive. In this project we will overcome these limitations, by developing the necessary algorithms to exploit new data sets that the PI has a major role in building,