The clustering of sub - mJy radio sources in The Bootes Deep Field

We measure the angular clustering of ∼ 2000 radio sources in The Bootes Deep Field, covering 5.3 deg 2 down to S 1.4GHz = 0.2 mJy. With reference to work by Blake & Wall, we show that the size distribution of multi-component radio galaxies dominates the overall clustering signal, and that its amplitude extrapolates smoothly from their measurements above 5 mJy. The upper limits on any true galaxy-galaxy clustering are consistent with the clustering of sub-mJy radio-loud AGN being effectively diluted by the more weakly-clustered IRAS-type starburst galaxies. Source count models imply that the survey contains ≃ 400 of the latter galaxies above 0.2 mJy out to z ∼ 1 − 2. Measurement of their clustering must await their identification via the optical and infrared data due on this field.