Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data.
- Submitting institution
-
University of Durham
- Unit of assessment
- 9 - Physics
- Output identifier
- 101152
- Type
- D - Journal article
- DOI
-
10.1093/mnras/stv1447
- Title of journal
- Monthly Notices of the Royal Astronomical Society
- Article number
- -
- First page
- 3529
- Volume
- 452
- Issue
- 4
- ISSN
- 00358711
- Open access status
- Out of scope for open access requirements
- Month of publication
- -
- Year of publication
- 2015
- URL
-
https://doi.org/10.1093/mnras/stv1447
- Supplementary information
-
-
- Request cross-referral to
- -
- Output has been delayed by COVID-19
- No
- COVID-19 affected output statement
- -
- Forensic science
- No
- Criminology
- No
- Interdisciplinary
- No
- Number of additional authors
-
26
- Research group(s)
-
D - Centre for Extragalactic Astronomy
- Citation count
- 84
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- I led the analysis of large-scale structure in the Galaxy and Mass Assembly (GAMA) survey. Viola et al. (2015) relies on my infrastructure work, including the modelling of the GAMA selection function, the construction of the GAMA group catalogue and the creation of GAMA mock galaxy catalogues constructed from large N-body simulations. Without these contributions this study would not have been possible. I played a central role in shaping and directing the analysis in Viola et al, and in the writing of the paper. This is reflected by my inclusion in the core author list, ahead of the alphabetized authors.
- Non-English
- No
- English abstract
- -
