Gaia17biu/SN 2017egm IN NGC 3191: THE CLOSEST HYDROGEN-POOR SUPERLUMINOUS SUPERNOVA TO DATE IS IN A \NORMAL", MASSIVE, METAL-RICH SPIRAL GALAXY
- Submitting institution
-
The University of Manchester
- Unit of assessment
- 9 - Physics
- Output identifier
- 63549461
- Type
- D - Journal article
- DOI
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10.3847/1538-4357/aaa298
- Title of journal
- The Astrophysical Journal
- Article number
- 57
- First page
- -
- Volume
- 853
- Issue
- 1
- ISSN
- 0004-637X
- Open access status
- Compliant
- Month of publication
- January
- Year of publication
- 2018
- 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
-
51
- Research group(s)
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A - Physics & Astro
- Citation count
- 30
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- Robert Beswick: Beswick was instrumental in obtaining, reducing and interpreting the radio observations presented in the work. These observations enabled the most stringent limits on the radio emission from Superluminous SNe and hence implications on the origins of these supernovae and how they relate to other types of SNe. Beswick, directly contributed to the science interpretation and writing of the publication and was the primary author of radio observation and data reduction sections.
- Non-English
- No
- English abstract
- -
