A continuum of H- to He-rich tidal disruption candidates with a preference for E+A galaxies
- Submitting institution
-
University of Southampton
- Unit of assessment
- 9 - Physics
- Output identifier
- 20498731
- Type
- D - Journal article
- DOI
-
10.1088/0004-637X/793/1/38
- Title of journal
- The Astrophysical Journal
- Article number
- -
- First page
- 1
- Volume
- 793
- Issue
- 38
- ISSN
- 0004-637X
- Open access status
- Out of scope for open access requirements
- Month of publication
- September
- 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
-
25
- Research group(s)
-
-
- Citation count
- 228
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- Mark Sullivan was third author on this paper; authors are listed in order of contribution to the paper. MS was responsible for i) all photometry for the events in the analysis (sec 2.1) which underpins the paper, including writing a custom photometry routine for this analysis; ii) performing the galaxy SED fitting and analysis (sec 3.3; 5.5), and iii) scientific interpretation and paper writing/editing.
- Non-English
- No
- English abstract
- -
