Properties of the binary neutron star merger GW170817
- Submitting institution
-
University of Glasgow
- Unit of assessment
- 9 - Physics
- Output identifier
- 9-08779
- Type
- D - Journal article
- DOI
-
10.1103/PhysRevX.9.011001
- Title of journal
- Physical Review X
- Article number
- 11001
- First page
- -
- Volume
- 9
- Issue
- 1
- ISSN
- 2160-3308
- Open access status
- Compliant
- Month of publication
- January
- Year of publication
- 2019
- URL
-
http://eprints.gla.ac.uk/177057/
- 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
-
1,147
- Research group(s)
-
-
- Citation count
- 346
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- I contributed to performing and validating the analysis reported here, including to interpretation of the results. I was a lead author of the software used in performing the parameter estimation. Further, as the co-leader of the group of scientists within the collaboration working directly on searches for gravitational waves from compact binary systems I was responsible for conceptualising and steering the overarching data analysis projects around GW170817, including defining goals for this paper.
- Non-English
- No
- English abstract
- -
