Herschel-ATLAS/GAMA: spatial clustering of low-redshift sub-mm galaxies
  We have measured the clustering properties of low-redshift (z < 0.3) sub-mm galaxies detected at 250 micron in the Herschel-ATLAS Science Demonstration Phase (SDP) field. We selected a sample for which we have high-quality spectroscopic redshifts, obtained from reliably matching the 250-micron sources to a complete (for r < 19.4) sample of galaxies from the GAMA database. Both the angular and spatial clustering strength are measured for all z < 0.3 sources as well as for five redshift slices with thickness delta z=0.05 in the range 0.05 < z < 0.3. Our measured spatial clustering length r_0 is comparable to that of optically-selected, moderately star-forming (blue) galaxies: we find values around 5 Mpc. One of the redshift bins contains an interesting structure, at z = 0.164. 
E. van Kampen, D. J. B. Smith, S. Maddox, A. M. Hopkins, I.   Valtchanov, J. A. Peacock, M. J. Michalowski, P. Norberg, S. E...
astro-ph.CO