Binaries: visual; Planetary systems; Planets and satellites: detection; Techniques: radial velocities; Direct imaging; Doppler measurement; Long-term trend; Main sequence stars; Orbital parameters; Planet search; Radial velocity; Southern Hemisphere; Astronomy and Astrophysics; Space and Planetary Science
Abstract :
[en] Context. Since 1998, a planet-search around main sequence stars within 50 pc in the southern hemisphere has been underway with the CORALIE spectrograph at La Silla Observatory. Aims. With an observing time span of more than 20 yr, the CORALIE survey is able to detect long-term trends in data with masses and separations large enough to select ideal targets for direct imaging. Detecting these giant companion candidates will allow us to start bridging the gap between radial-velocity-detected exoplanets and directly imaged planets and brown dwarfs. Methods. Long-term precise Doppler measurements with the CORALIE spectrograph reveal radial-velocity signatures of massive planetary companions and brown dwarfs on long-period orbits. Results. In this paper, we report the discovery of new companions orbiting HD 181234, HD 13724, HD 25015, HD 92987 and HD 50499. We also report updated orbital parameters for HD 50499b, HD 92788b and HD 98649b. In addition, we confirm the recent detection of HD 92788c. The newly reported companions span a period range of 15.6-40.4 yr and a mass domain of 2.93-26.77 MJup, the latter of which straddles the nominal boundary between planets and brown dwarfs. Conclusions. We report the detection of five new companions and updated parameters of four known extrasolar planets. We identify at least some of these companions to be promising candidates for imaging and further characterisation.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Rickman, E.L.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Ségransan, D.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Marmier, M.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Udry, S.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Bouchy, F.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Lovis, C.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Mayor, M.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Pepe, F.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Queloz, D.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Santos, N.C.; Instituto de Astrofísica e Ciências Do Espaço, Universidade Do Porto, Caup, Porto, Portugal ; Departamento de Física e Astronomia, Faculdade de Ciências, Universidade Do Porto, Porto, Portugal
Allart, R.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Bonvin, V.; Institute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, Versoix, Switzerland
Bratschi, P.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Cersullo, F.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Chazelas, B.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Choplin, A.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Conod, U.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Deline, A.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Delisle, J.-B.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Dos Santos, L.A.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Figueira, P.; Instituto de Astrofísica e Ciências Do Espaço, Universidade Do Porto, Caup, Porto, Portugal ; European Southern Observatory, Vitacura, Santiago, Chile
Giles, H.A.C.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Girard, M.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Lavie, B.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Martin, D.; Département d'Astronomie, Université de Genève, Versoix, Switzerland ; Department of Astronomy and Astrophysics, University of Chicago, Chicago, United States
Motalebi, F.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Nielsen, L.D.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Osborn, H.; Department of Physics, University of Warwick, Coventry, United Kingdom ; Aix Marseille Université, Cnrs, Lam (Laboratoire d'Astrophysique de Marseille) Umr 7326, Marseille, France
Ottoni, G.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Raimbault, M.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Rey, J.; Département d'Astronomie, Université de Genève, Versoix, Switzerland ; Carnegie Institution for Science, Las Campanas Observatory, Casilla 601, La Serena, Chile
Roger, T.; Département d'Astronomie, Université de Genève, Versoix, Switzerland ; Physikalisches Institut, Universität Bern, Bern, Switzerland
Seidel, J.V.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Stalport, Manu ; Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR) ; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Suárez Mascareño, A.; Département d'Astronomie, Université de Genève, Versoix, Switzerland ; Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
Triaud, A.; School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, United Kingdom
Turner, O.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Weber, L.; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Wyttenbach, A.; Département d'Astronomie, Université de Genève, Versoix, Switzerland ; Leiden Observatory, Leiden University, Leiden, Netherlands
Acknowledgements. This work has been carried out within the framework of the National Centre for Competence in Research PlanetS supported by the Swiss National Science Foundation. The authors acknowledge the financial support of the SNSF. This publication makes use of the Data & Analysis Center for Exoplanets (DACE), which is a facility based at the University of Geneva (CH) dedicated to extrasolar planets data visualisation, exchange and analysis. DACE is a platform of the Swiss National Centre of Competence in Research (NCCR) PlanetS, federating the Swiss expertise in Exoplanet research. The DACE platform is available at https://dace.unige.ch. L.A.dS. and J.V.S. acknowledge the support from the European Research Council (ERC) under the European Union\u2019s Horizon 2020 research and innovation programme (project FOUR ACES, grant agreement No 724427). N.C.S. was supported by FCT \u2013 Funda\u00E7\u00E3o para a Ci\u00EAncia e a Tecnologia \u2013 through national funds and by FEDER through COMPETE2020 \u2013 Programa Operacional Competitividade e Internacionaliza\u00E7\u00E3o by these grants: UID/FIS/04434/2013 & POCI-01-0145-FEDER-007672; PTDC/FIS-AST/28953/2017 & POCI-01-0145-FEDER-028953 and PTDC/FIS-AST/32113/2017 & POCI-01-0145-FEDER-032113. This work has made use of data from the European Space Agency (ESA) mission Gaia (http://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, http://www.cosmos.esa.int/web/ gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.
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