Journal Article

<i>Herschel</i>-ATLAS/GAMA: spatial clustering of low-redshift submm galaxies

E. van Kampen, D. J. B. Smith, S. Maddox, A. M. Hopkins, I. Valtchanov, J. A. Peacock, M. J. Michałowski, P. Norberg, S. Eales, L. Dunne, J. Liske, M. Baes, D. Scott, E. Rigby, A. Robotham, P. van der Werf, E. Ibar, M. J. Jarvis, J. Loveday, R. Auld, I. K. Baldry, S. Bamford, E. Cameron, S. Croom, S. Buttiglione, A. Cava, A. Cooray, S. Driver, J. S. Dunlop, A. Dariush, J. Fritz, R. J. Ivison, E. Pascale, M. Pohlen, G. Rodighiero, P. Temi, D. G. Bonfield, D. Hill, D. H. Jones, L. Kelvin, H. Parkinson, M. Prescott, R. Sharp, G. de Zotti, S. Serjeant, C. C. Popescu and R. J. Tuffs

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 426, issue 4, pages 3455-3463
Published in print November 2012 | ISSN: 0035-8711
Published online November 2012 | e-ISSN: 1365-2966 | DOI:
Herschel-ATLAS/GAMA: spatial clustering of low-redshift submm galaxies

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We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 μm in the Herschel-ATLAS science demonstration phase field. We selected a sample for which we have high-quality spectroscopic redshifts, obtained from reliably matching the 250-μm sources to a complete (for r < 19.4) sample of galaxies from the GAMA data base. Both the angular and spatial clustering strength are measured for all z < 0.3 sources as well as for five redshift slices with thickness Δz = 0.05 in the range 0.05 < z < 0.3. Our measured spatial clustering length r0 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.

Keywords: surveys; galaxies: statistics; large-scale structure of Universe; submillimetre: galaxies

Journal Article.  5558 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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