Journal
ASTRONOMY & ASTROPHYSICS
Volume 518, Issue -, Pages -Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361/201014597
Keywords
submillimeter: galaxies; large-scale structure of Universe; cosmology: observations; galaxies: evolution; galaxies: high-redshift
Categories
Funding
- NASA
- CSA (Canada)
- NAOC (China)
- CEA (France)
- CNES (France)
- CNRS (France)
- ASI (Italy)
- MCINN (Spain)
- SNSB (Sweden)
- STFC (UK)
- NASA (USA)
- STFC [ST/G002630/1, ST/F007019/1, ST/F002858/1, PP/E005306/1, ST/H001530/1, PP/E001173/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/G002630/1, ST/F002858/1, PP/E001181/1, PP/E005306/1, ST/F007019/1, PP/E001173/1] Funding Source: researchfish
- UK Space Agency [ST/G003874/1] Funding Source: researchfish
Ask authors/readers for more resources
We measure the angular correlation function, omega(theta), from 0.5 to 30 arcmin of detected sources in two wide fields of the Herschel Multi-tiered Extragalactic Survey (HerMES). Our measurements are consistent with the expected clustering shape from a population of sources that trace the dark matter density field, including non-linear clustering at arcminute angular scales arising from multiple sources that occupy the same dark matter halos. By making use of the halo model to connect the spatial clustering of sources to the dark matter halo distribution, we estimate source bias and halo occupation number for dusty sub-mm galaxies at z similar to 2. We find that sub-mm galaxies with 250 mu m flux densities above 30 mJy reside in dark matter halos with mass above (5 +/- 4) x 10(12) M-circle dot, while (14 +/- 8)% of such sources appear as satellites in more massive halos.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available