- Abstract:
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We study the stellar-to-halo mass relation of central galaxies in the range 9.7 < log10(M*/h-2 M⊙) < 11.7 and z < 0.4, obtained from a combined analysis of the Kilo Degree Survey (KiDS) and the Galaxy And Mass Assembly (GAMA) survey. We use ~100 deg2 of KiDS data to study the lensing signal around galaxies for which spectroscopic redshifts and stellar masses were determined by GAMA. We show that lensing alone results in poor constraints on the stellar-to-halo mass relation due to a d...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 1.6MB)
-
- Publisher copy:
- 10.1093/mnras/stw747
-
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- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 459
- Issue:
- 3
- Pages:
- 3251-3270
- Publication date:
- 2016-04-12
- DOI:
- EISSN:
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1365-2966
- ISSN:
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0035-8711
- Pubs id:
-
pubs:630898
- URN:
-
uri:2af1b8e1-1e78-4363-8fa2-5d523c177e4e
- UUID:
-
uuid:2af1b8e1-1e78-4363-8fa2-5d523c177e4e
- Local pid:
- pubs:630898
- Paper number:
- 3
- Copyright holder:
- van Uitert et al.
- Copyright date:
- 2016
- Notes:
- © 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
Journal article
The stellar-to-halo mass relation of GAMA galaxies from 100 deg 2 of KiDS weak lensing data
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