A temperate rocky super-Earth transiting a nearby cool star
- Submitting institution
-
University of Exeter
- Unit of assessment
- 9 - Physics
- Output identifier
- 6500
- Type
- D - Journal article
- DOI
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10.1038/nature22055
- Title of journal
- Nature
- Article number
- -
- First page
- 333
- Volume
- 544
- Issue
- 7650
- ISSN
- 0028-0836
- Open access status
- Deposit exception
- Month of publication
- April
- Year of publication
- 2017
- 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
- 170
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- Haywood measured the mass of the planet by applying Gaussian regression analysis to the radial-velocity observations. This technique accounts for the correlated noise arising from the intrinsic variability of the host star, yielding an accurate planetary mass determination. She also contributed to the generation of figures and writing of the paper.
- Non-English
- No
- English abstract
- -