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Cited by 66Stellar, planetary, and galactic studiesAstronomy and Astrophysical ResearchAstro and Planetary Science

The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.

New planetary systems from the Calan–Hertfordshire Extrasolar Planet Search

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Jenkins, J. S., Jones, H. R. A., Tuomi, M., Díaz, M., Cordero, J. P., Aguayo, A., Pantoja, B., Arriagada, P., Mahu, R., Brahm, R., Rojo, P., Soto, M. G., Ivanyuk, O., Becerra Yoma, N., Day-Jones, A. C., Ruiz, M. T., Pavlenko, Y. V., Barnes, J. R., Murgas, F., Pinfield, D. J., Jones, M. I., López-Morales, M., Shectman, S., Butler, R. P., Minniti, D.·2017·Monthly Notices of the Royal Astronomical Society
DOI 10.1093/mnras/stw2811
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Abstract

We report the discovery of eight new giant planets, and updated orbits for four known planets, orbiting dwarf and subgiant stars using the CORALIE, HARPS, and MIKE instruments as part of the Calan-Hertfordshire Extrasolar Planet Search.The planets have masses in the range 1.1-5.4M J 's, orbital periods from 40 to 2900 d, and eccentricities from 0.0 to 0.6.They include a double-planet system orbiting the most massive star in our sample (HD147873), two eccentric giant planets (HD128356b and HD154672b), and a rare 14 Herculis analogue (HD224538b).We highlight some population correlations from the sample of radial velocity detected planets orbiting nearby stars, including the mass function exponential distribution, confirmation of the growing body of evidence that low-mass planets tend to be found orbiting more metal-poor stars than giant planets, and a possible period-metallicity correlation for planets with masses >0.1 M J , based on a metallicity difference of 0.16 dex between the population of planets with orbital periods less than 100 d and those with orbital periods greater than 100 d.

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  • Observationally, there is some evidence for a further enhancement of hot Jupiters relative to cold Jupiters at higher host star metallicities.

    “Observationally, there is some evidence for a further enhancement of hot Jupiters relative to cold Jupiters at higher host star metallicities.”

    From Origins of Hot Jupiters (2018) · cites this paper as Jenkins et al. (2017)

  • Jenkins et al. (2017) found that giant planets with orbital periods less than 100 days orbit more metal rich stars than giant planets with orbital periods greater than 100 days.

    “Jenkins et al. (2017) found that giant planets with orbital periods less than 100 days orbit more metal rich stars than giant planets with orbital periods greater than 100 days.”

    From Origins of Hot Jupiters (2018) · cites this paper as Jenkins et al. (2017)

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Cites

  • No planet for HD 166435

    Queloz, D., Henry, G. W., Sivan, J. P., Baliunas, S. L., Beuzit, J. L., Donahue, R. A., Mayor, M., Naef, D., Perrier, C., & Udry, S. (2001) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20011308 · Cited by 913 · cited 2×

    “The BIS values for HARPS were taken from the HARPS-DRS and measured following the method explained in Queloz et al. (2001).”
    BackgroundMethod

  • An Earth-mass planet orbiting α Centauri B

    Dumusque, X., Pepe, F., Lovis, C., Ségransan, D., Sahlmann, J., Benz, W., Bouchy, F., Mayor, M., Queloz, D., Santos, N., et al. (2012) · Nature · doi:10.1038/nature11572 · Cited by 404 · cited 1×

    “…lowest mass planet in the high metallicity sample, neglecting the exceptional case MNRAS 000, 1–20 (2002) of the planet orbiting Alpha Centauri B (Dumusque et al. 2012) that Hatzes (2013) and Rajpaul et al. (2015) claim may be attributed to other phenomena like stellar activity or sampling…”
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Metadata

Authors
Jenkins, J. S., Jones, H. R. A., Tuomi, M., Díaz, M., Cordero, J. P., Aguayo, A., Pantoja, B., Arriagada, P., Mahu, R., Brahm, R., Rojo, P., Soto, M. G., Ivanyuk, O., Becerra Yoma, N., Day-Jones, A. C., Ruiz, M. T., Pavlenko, Y. V., Barnes, J. R., Murgas, F., Pinfield, D. J., Jones, M. I., López-Morales, M., Shectman, S., Butler, R. P., & Minniti, D.
Affiliations
  • University of Chile (CL)
  • University of Hertfordshire (GB)
  • Carnegie Institution for Science (US)
  • Pontificia Universidad Católica de Chile (CL)
  • Main Astronomical Observatory (UA)
  • The Open University (GB)
  • Instituto de Astrofísica de Canarias (ES)
  • Universidad Andrés Bello (CL)
Corresponding author
Jenkins, J. S.
ORCID
Venue
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press (OUP)
Published
2016-11-02
Volume
466
Issue
1
Pages
443-473
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
DOI
10.1093/mnras/stw2811
OpenAlex
W2548132265
Cited by
66
References
2
Citations by year
2026: 2 · 2025: 3 · 2024: 6 · 2023: 4 · 2022: 7 · 2021: 4 · 2020: 7 · 2019: 12 · 2018: 14 · 2017: 7
FWCI
5.26
Type
journal article
Language
en
Open access
Locations
  • Monthly Notices of the Royal Astronomical Society (publishedVersion)
  • Open Research Online - ORO (The Open University) (acceptedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • University of Hertfordshire Research Archive (University of Hertfordshire) (submittedVersion)
  • Universidad de Chile (submittedVersion, cc-by-nc-nd)
  • Repositorio Institucional Académico , Sistema de Bibliotecas Universidad Andrés Bello (UNAB) (Universidad Andrés Bello (UNAB)) (submittedVersion)
  • arXiv (Cornell University)
Funders
CATA (PFB-06)
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 › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
Keywords
exoplanets, giant planets, radial velocity, mass function, metallicity, orbital eccentricity, CORALIE, HARPS, Mike

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