Properties of the binary black hole merger GW150914
- Submitting institution
-
Cardiff University / Prifysgol Caerdydd
- Unit of assessment
- 9 - Physics
- Output identifier
- 96758330
- Type
- D - Journal article
- DOI
-
10.1103/PhysRevLett.116.241102
- Title of journal
- Physical Review Letters
- Article number
- 241102
- First page
- -
- Volume
- 116
- Issue
- 24
- ISSN
- 0031-9007
- Open access status
- Compliant
- Month of publication
- June
- Year of publication
- 2016
- URL
-
http://dx.doi.org/10.1103/PhysRevLett.116.241102
- 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
-
976
- Research group(s)
-
G - Gravitational Physics
- Citation count
- 699
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- I produced the generic binary waveform model used to measure the parameters of the source. This was the only model that included all measurable physical effects in the signal, and was therefore crucial to measuring the properties of the first gravitational-wave detection. I also contributed to the analysis, and to the writing of all sections of the paper.
- Non-English
- No
- English abstract
- -
