An ultraluminous X-ray source powered by an accreting neutron star.
- Submitting institution
-
University of Cambridge
- Unit of assessment
- 9 - Physics
- Output identifier
- 6711
- Type
- D - Journal article
- DOI
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10.1038/nature13791
- Title of journal
- Nature
- Article number
- -
- First page
- 202
- Volume
- 514
- Issue
- 7521
- ISSN
- 1476-4687
- Open access status
- Out of scope for open access requirements
- Month of publication
- October
- Year of publication
- 2014
- 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
-
23
- Research group(s)
-
-
- Citation count
- 368
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- Walton led the analysis of imaging data from the Chandra X-ray Observatory and NuSTAR observatory. They found the on-pulse/off-pulse shift of centroid of the NuSTAR emission which was pivotal in correctly assigning the pulses to the ultraluminous X-ray source. They were closely involved in the writing of the paper.
- Non-English
- No
- English abstract
- -
