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HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements

Abstract:

We measure the angular correlation function, w(θ), 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 cl...

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Publisher copy:
10.1051/0004-6361/201014597

Authors


Amblard, A More by this author
Arumugam, V More by this author
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Journal:
Astronomy and Astrophysics
Volume:
518
Issue:
1
Publication date:
2010-07-16
DOI:
EISSN:
1432-0746
ISSN:
0004-6361
URN:
uuid:77fd8dae-32e0-454a-9b9e-584ca2c85bde
Source identifiers:
202830
Local pid:
pubs:202830

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