The DOI matches its Crossref record; 34 of the 34 references it cites were found in a registry or an index.
Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b
Open accessAbstract
We report the discovery of the transiting exoplanets WASP-95b, WASP-96b, WASP-97b, WASP-98b, WASP-99b, WASP-100b and WASP-101b. All are hot Jupiters with orbital periods in the range 2.1–5.7 d, masses of 0.5–2.8 MJup and radii of 1.1–1.4 RJup. The orbits of all the planets are compatible with zero eccentricity. WASP-99b produces the shallowest transit yet found by WASP-South, at 0.4 per cent. The host stars are of spectral type F2–G8. Five have metallicities of [Fe/H] from −0.03 to +0.23, while WASP-98 has a metallicity of −0.60, exceptionally low for a star with a transiting exoplanet. Five of the host stars are brighter than V = 10.8, which significantly extends the number of bright transiting systems available for follow-up studies. WASP-95 shows a possible rotational modulation at a period of 20.7 d. We discuss the completeness of WASP survey techniques by comparing to the HATnet project.
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Metadata
- Authors
- Hellier, C., Anderson, D. R., Cameron, A. C., Delrez, L., Gillon, M., Jehin, E., Lendl, M., Maxted, P. F. L., Pepe, F., Pollacco, D., Queloz, D., Ségransan, D., Smalley, B., Smith, A. M. S., Southworth, J., Triaud, A. H. M. J., Udry, S., & West, R. G.
- Affiliations
- Keele University (GB)
- University of St Andrews (GB)
- University of Liège (BE)
- University of Geneva (CH)
- University of Warwick (GB)
- Nicolaus Copernicus Astronomical Center (PL)
- Corresponding author
- Hellier, Coel
- ORCID
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2014-04-03
- Volume
- 440
- Issue
- 3
- Pages
- 1982-1992
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W1985958802
- Cited by
- 135
- References
- 34
- Citations by year
- 2026: 7 · 2025: 9 · 2024: 14 · 2023: 18 · 2022: 9 · 2021: 8 · 2020: 8 · 2019: 9 · 2018: 29 · 2017: 10 · 2016: 7 · 2015: 2 · 2014: 3
- FWCI
- 3.95
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Monthly Notices of the Royal Astronomical Society (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Keele Research Repository (Keele University) (submittedVersion, cc-by)
- ORBi (University of Liège) (submittedVersion, other-oa)
- St Andrews Research Repository (St Andrews Research Repository) (submittedVersion)
- University of Birmingham Research Portal (University of Birmingham) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Science Foundation
- Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung (145594)
- Fonds De La Recherche Scientifique - FNRS (FRFC 2.5.594.09)
- Science and Technology Facilities Council (ST/K006126/1, ST/L000733/1, ST/J00152X/1, PP/F000065/1, PP/F000073/1, ST/J001651/1, ST/H005307/1, ST/I001719/1)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › History and Developments in Astronomy
- Keywords
- hot Jupiters, transiting exoplanets, Trappists, host star metallicity, survey completeness
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