Herschel-ATLAS/GAMA: spatial clustering of low-redshift submm galaxies
| Autor: | A. Dariush, Steve Eales, Scott M. Croom, Matt J. Jarvis, G. Rodighiero, Maarten Baes, G. de Zotti, R. J. Tuffs, Pasquale Temi, I. Valtchanov, Ivan K. Baldry, Douglas Scott, Rob Ivison, L. Kelvin, Denis Hill, D. J. B. Smith, Michał J. Michałowski, Cristina Popescu, David Bonfield, Steve Serjeant, R. G. Sharp, Loretta Dunne, John A. Peacock, Robbie Richard Auld, James Dunlop, Enzo Pascale, Jochen Liske, S. Buttiglione, Ewan Cameron, E. Ibar, S. J. Maddox, Steven P. Bamford, Simon P. Driver, E. E. Rigby, Antonio Cava, H. Parkinson, Jacopo Fritz, P. van der Werf, Asantha Cooray, E. van Kampen, D. H. P. Jones, M. Pohlen, Jonathan Loveday, Matthew Prescott, Aaron S. G. Robotham, Peder Norberg, Andrew M. Hopkins |
|---|---|
| Rok vydání: | 2012 |
| Předmět: |
Physics
Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics 01 natural sciences Galaxy Redshift medicine.anatomical_structure Space and Planetary Science Atlas (anatomy) 0103 physical sciences medicine Spatial clustering 010306 general physics Cluster analysis 010303 astronomy & astrophysics Astrophysics::Galaxy Astrophysics |
| Zdroj: | Monthly Notices of the Royal Astronomical Society. 426:3455-3463 |
| ISSN: | 0035-8711 |
| Popis: | 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. |
| Databáze: | OpenAIRE |
| Externí odkaz: |
|
Plný text