Gravitational waves from binary supermassive black holes missing in pulsar observations
- Submitting institution
-
The University of Manchester
- Unit of assessment
- 9 - Physics
- Output identifier
- 51382374
- Type
- D - Journal article
- DOI
-
10.1126/science.aab1910
- Title of journal
- Science
- Article number
- -
- First page
- 1522
- Volume
- 349
- Issue
- 6255
- ISSN
- 0036-8075
- Open access status
- Out of scope for open access requirements
- Month of publication
- September
- Year of publication
- 2015
- 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
-
21
- Research group(s)
-
A - Physics & Astro
- Citation count
- 228
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- Michael Keith: The pulsar observations which directly underpin this paper are a long-term monitoring effort to which Keith contributed by performing a significant fraction of the observations. As a member of the science executive board of the consortium at the time, he helped design the most efficient observing strategy. He also contributed to the data analysis and interpretation of results presented in the paper. In particular, he looked at the contribution of the timing noise to the overall quality of the timing and discussed their implication for the limit on the presented limit on the detection of gravitational waves.
- Non-English
- No
- English abstract
- -
