- Abstract:
-
Quantifying how the baryonic matter traces the underlying dark matter distribution is key to both understanding galaxy formation and our ability to constrain the cosmological model. Using the cross-correlation function of radio and near-infrared galaxies, we present a large-scale clustering analysis of radio galaxies to z ~ 2.2. We measure the angular auto-correlation function of Ks<23.5 galaxies in the VISTA Deep Extragalactic Observations (VIDEO-XMM3) field with photometric redshifts out...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1093/mnras/stu453
-
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- Publisher:
- Blackwell Publishing Ltd
- Journal:
- MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Volume:
- 440
- Issue:
- 3
- Pages:
- 2322-2332
- Publication date:
- 2014-05-05
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:be76fd38-2a4b-4284-ad3d-94e5448f4195
- Source identifiers:
-
464659
- Local pid:
- pubs:464659
- Language:
- English
- Keywords:
- Copyright date:
- 2014
Journal article
Evolution in the bias of faint radio sources to z similar to 2.2
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