GRB 130925A: an ultralong gamma ray burst with a dust-echo afterglow, and implications for the origin of the ultralong GRBs
- Submitting institution
-
The University of Leicester
- Unit of assessment
- 9 - Physics
- Output identifier
- 1976
- Type
- D - Journal article
- DOI
-
10.1093/mnras/stu1459
- Title of journal
- Monthly Notices of the Royal Astronomical Society
- Article number
- -
- First page
- 250
- Volume
- 444
- Issue
- 1
- ISSN
- 0035-8711
- Open access status
- Out of scope for open access requirements
- Month of publication
- August
- Year of publication
- 2014
- URL
-
-
- Supplementary information
-
https://doi.org/10.1093/mnras/stu1459
- 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
-
26
- Research group(s)
-
-
- Citation count
- 47
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- R. Willingale was responsible for the main tenet of the paper. He devised the dust-echo model, set up the software to fit the model to the data and performed the data analysis. He generated most of the material in sections 3 and 4 which describe the considerable details of the modelling and fitting procedures. He produced the many figures that illustrate the model and results, in particular, the best fitting parameters for the 38 pulses listed in table 6 the dust model results in Table 7.
- Non-English
- No
- English abstract
- -
