LoCuSS : scaling relations between galaxy cluster mass, gas, and stellar content
- Submitting institution
-
The University of Birmingham
- Unit of assessment
- 9 - Physics
- Output identifier
- 83646792
- Type
- D - Journal article
- DOI
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10.1093/mnras/sty3484
- Title of journal
- Monthly Notices of the Royal Astronomical Society
- Article number
- -
- First page
- 60
- Volume
- 484
- Issue
- 1
- ISSN
- 0035-8711
- Open access status
- Not compliant
- Month of publication
- January
- Year of publication
- 2019
- URL
-
-
- 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
-
15
- Research group(s)
-
-
- Citation count
- 13
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- In this paper, McGee contributed to the determination of the optical properties of the clusters by measuring the Brightest Cluster Galaxy luminosities through profile fitting and contributing to the code for the calculation of the optical richness. He also contributed to several parts of the interpretation of the paper, including writing portions of the discussion. He was deeply involved in the testing of the hierarchical Bayesian method, and the comparison to other methods in the literature.
- Non-English
- No
- English abstract
- -