The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits
- Autores
- Demangeon, O. D. S.; Dalal, S.; Hébrard, G.; Nsamba, B.; Kiefer, F.; Camacho, J.D.; Sahlmann, J.; Arnold, L.; Astudillo Defru, Nicola; Bonfils, X.; Boisse, I.; Bouchy, F.; Bourrier, V.; Campante, T.; Delfosse, X.; Deleuil, M.; Diaz, Rodrigo Fernando; Faria, J.; Forveille, T.; Hara, N.; Heidari, N.; Hobson, M.J.; Lopez, T.; Moutou, C.; Rey, J.; Santerne, A.; Sousa, S.; Santos, N. C.; Strøm, P. A.; Tsantaki, M.; Udry, S.
- Año de publicación
- 2021
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Context. Due to their low transit probability, the long-period planets are, as a population, only partially probed by transit surveys. Radial velocity surveys thus have a key role to play, in particular for giant planets. Cold Jupiters induce a typical radial velocity semi-amplitude of 10 m s-1, which is well within the reach of multiple instruments that have now been in operation for more than a decade. Aims. We take advantage of the ongoing radial velocity survey with the » SOPHIE high-resolution spectrograph, which continues the search started by its predecessor » ELODIE to further characterize the cold Jupiter population. Methods. Analyzing the radial velocity data from six bright solar-like stars taken over a period of up to 15 yr, we attempt the detection and confirmation of Keplerian signals. Results. We announce the discovery of six planets, one per system, with minimum masses in the range 4.8-8.3 Mjup and orbital periods between 200 days and 10 yr. The data do not provide enough evidence to support the presence of additional planets in any of these systems. The analysis of stellar activity indicators confirms the planetary nature of the detected signals. Conclusions. These six planets belong to the cold and massive Jupiter population, and four of them populate its eccentric tail. In this respect, HD 80869 b stands out as having one of the most eccentric orbits, with an eccentricity of 0.862-0.018+0.028. These planets can thus help to better constrain the migration and evolution processes at play in the gas giant population. Furthermore, recent works presenting the correlation between small planets and cold Jupiters indicate that these systems are good candidates to search for small inner planets.
Fil: Demangeon, O. D. S.. Universidad de Porto; Portugal
Fil: Dalal, S.. Institut d'Astrophysique de Paris; Francia
Fil: Hébrard, G.. Institut d'Astrophysique de Paris; Francia. Université d’Aix-Marseille; Francia
Fil: Nsamba, B.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania. Mbarara University of Science and Technology; Uganda. Universidad de Porto; Portugal
Fil: Kiefer, F.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Institut d'Astrophysique de Paris; Francia. Sorbonne University; Francia
Fil: Camacho, J.D.. Universidad de Porto; Portugal
Fil: Sahlmann, J.. European Space Astronomy Centre; España
Fil: Arnold, L.. Université d’Aix-Marseille; Francia
Fil: Astudillo Defru, Nicola. Universidad Católica de la Santísima Concepción; Chile
Fil: Bonfils, X.. Universite Grenoble Alpes; Francia
Fil: Boisse, I.. Université d’Aix-Marseille; Francia
Fil: Bouchy, F.. Universidad de Ginebra; Suiza
Fil: Bourrier, V.. Universidad de Ginebra; Suiza
Fil: Campante, T.. Universidad de Porto; Portugal
Fil: Delfosse, X.. Universite Grenoble Alpes; Francia
Fil: Deleuil, M.. Université d’Aix-Marseille; Francia
Fil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Ciencias Físicas. - Universidad Nacional de San Martín. Instituto de Ciencias Físicas; Argentina. Universidad Nacional de San Martín. Escuela de Política y Gobierno; Argentina
Fil: Faria, J.. Universidad de Porto; Portugal
Fil: Forveille, T.. Universite Grenoble Alpes; Francia
Fil: Hara, N.. Universidad de Ginebra; Suiza
Fil: Heidari, N.. Université Nice Sophia Antipolis. Laboratoire Joseph-louis Lagrange; Francia. Shahid Beheshti University; Irán. Université d’Aix-Marseille; Francia
Fil: Hobson, M.J.. Instituto Milenio de Astrofísica; Chile. Pontificia Universidad Católica de Chile; Chile
Fil: Lopez, T.. Université d’Aix-Marseille; Francia
Fil: Moutou, C.. Universite de Toulose - Le Mirail; Francia
Fil: Rey, J.. Carnegie Institution of Washington. Las Campanas Observatory; Chile
Fil: Santerne, A.. Université d’Aix-Marseille; Francia
Fil: Sousa, S.. Universidad de Porto; Portugal
Fil: Santos, N. C.. Universidad de Porto; Portugal
Fil: Strøm, P. A.. Sorbonne University; Francia. University of Warwick; Reino Unido
Fil: Tsantaki, M.. Osservatorio Astrofisico Di Arcetri; Italia. Universidad de Porto; Portugal
Fil: Udry, S.. Universidad de Ginebra; Suiza - Materia
-
PLANETS AND SATELLITES: DETECTION
TECHNIQUES: RADIAL VELOCITIES - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/154526
Ver los metadatos del registro completo
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The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbitsDemangeon, O. D. S.Dalal, S.Hébrard, G.Nsamba, B.Kiefer, F.Camacho, J.D.Sahlmann, J.Arnold, L.Astudillo Defru, NicolaBonfils, X.Boisse, I.Bouchy, F.Bourrier, V.Campante, T.Delfosse, X.Deleuil, M.Diaz, Rodrigo FernandoFaria, J.Forveille, T.Hara, N.Heidari, N.Hobson, M.J.Lopez, T.Moutou, C.Rey, J.Santerne, A.Sousa, S.Santos, N. C.Strøm, P. A.Tsantaki, M.Udry, S.PLANETS AND SATELLITES: DETECTIONTECHNIQUES: RADIAL VELOCITIEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. Due to their low transit probability, the long-period planets are, as a population, only partially probed by transit surveys. Radial velocity surveys thus have a key role to play, in particular for giant planets. Cold Jupiters induce a typical radial velocity semi-amplitude of 10 m s-1, which is well within the reach of multiple instruments that have now been in operation for more than a decade. Aims. We take advantage of the ongoing radial velocity survey with the » SOPHIE high-resolution spectrograph, which continues the search started by its predecessor » ELODIE to further characterize the cold Jupiter population. Methods. Analyzing the radial velocity data from six bright solar-like stars taken over a period of up to 15 yr, we attempt the detection and confirmation of Keplerian signals. Results. We announce the discovery of six planets, one per system, with minimum masses in the range 4.8-8.3 Mjup and orbital periods between 200 days and 10 yr. The data do not provide enough evidence to support the presence of additional planets in any of these systems. The analysis of stellar activity indicators confirms the planetary nature of the detected signals. Conclusions. These six planets belong to the cold and massive Jupiter population, and four of them populate its eccentric tail. In this respect, HD 80869 b stands out as having one of the most eccentric orbits, with an eccentricity of 0.862-0.018+0.028. These planets can thus help to better constrain the migration and evolution processes at play in the gas giant population. Furthermore, recent works presenting the correlation between small planets and cold Jupiters indicate that these systems are good candidates to search for small inner planets.Fil: Demangeon, O. D. S.. Universidad de Porto; PortugalFil: Dalal, S.. Institut d'Astrophysique de Paris; FranciaFil: Hébrard, G.. Institut d'Astrophysique de Paris; Francia. Université d’Aix-Marseille; FranciaFil: Nsamba, B.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania. Mbarara University of Science and Technology; Uganda. Universidad de Porto; PortugalFil: Kiefer, F.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Institut d'Astrophysique de Paris; Francia. Sorbonne University; FranciaFil: Camacho, J.D.. Universidad de Porto; PortugalFil: Sahlmann, J.. European Space Astronomy Centre; EspañaFil: Arnold, L.. Université d’Aix-Marseille; FranciaFil: Astudillo Defru, Nicola. Universidad Católica de la Santísima Concepción; ChileFil: Bonfils, X.. Universite Grenoble Alpes; FranciaFil: Boisse, I.. Université d’Aix-Marseille; FranciaFil: Bouchy, F.. Universidad de Ginebra; SuizaFil: Bourrier, V.. Universidad de Ginebra; SuizaFil: Campante, T.. Universidad de Porto; PortugalFil: Delfosse, X.. Universite Grenoble Alpes; FranciaFil: Deleuil, M.. Université d’Aix-Marseille; FranciaFil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Ciencias Físicas. - Universidad Nacional de San Martín. Instituto de Ciencias Físicas; Argentina. Universidad Nacional de San Martín. Escuela de Política y Gobierno; ArgentinaFil: Faria, J.. Universidad de Porto; PortugalFil: Forveille, T.. Universite Grenoble Alpes; FranciaFil: Hara, N.. Universidad de Ginebra; SuizaFil: Heidari, N.. Université Nice Sophia Antipolis. Laboratoire Joseph-louis Lagrange; Francia. Shahid Beheshti University; Irán. Université d’Aix-Marseille; FranciaFil: Hobson, M.J.. Instituto Milenio de Astrofísica; Chile. Pontificia Universidad Católica de Chile; ChileFil: Lopez, T.. Université d’Aix-Marseille; FranciaFil: Moutou, C.. Universite de Toulose - Le Mirail; FranciaFil: Rey, J.. Carnegie Institution of Washington. Las Campanas Observatory; ChileFil: Santerne, A.. Université d’Aix-Marseille; FranciaFil: Sousa, S.. Universidad de Porto; PortugalFil: Santos, N. C.. Universidad de Porto; PortugalFil: Strøm, P. A.. Sorbonne University; Francia. University of Warwick; Reino UnidoFil: Tsantaki, M.. Osservatorio Astrofisico Di Arcetri; Italia. Universidad de Porto; PortugalFil: Udry, S.. Universidad de Ginebra; SuizaEDP Sciences2021-09-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/154526Demangeon, O. D. S.; Dalal, S.; Hébrard, G.; Nsamba, B.; Kiefer, F.; et al.; The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits; EDP Sciences; Astronomy and Astrophysics; 653; A78; 10-9-2021; 1-240004-63611432-0746CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202141079info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2021/09/aa41079-21/aa41079-21.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:38:04Zoai:ri.conicet.gov.ar:11336/154526instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:38:04.749CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits |
| title |
The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits |
| spellingShingle |
The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits Demangeon, O. D. S. PLANETS AND SATELLITES: DETECTION TECHNIQUES: RADIAL VELOCITIES |
| title_short |
The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits |
| title_full |
The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits |
| title_fullStr |
The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits |
| title_full_unstemmed |
The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits |
| title_sort |
The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits |
| dc.creator.none.fl_str_mv |
Demangeon, O. D. S. Dalal, S. Hébrard, G. Nsamba, B. Kiefer, F. Camacho, J.D. Sahlmann, J. Arnold, L. Astudillo Defru, Nicola Bonfils, X. Boisse, I. Bouchy, F. Bourrier, V. Campante, T. Delfosse, X. Deleuil, M. Diaz, Rodrigo Fernando Faria, J. Forveille, T. Hara, N. Heidari, N. Hobson, M.J. Lopez, T. Moutou, C. Rey, J. Santerne, A. Sousa, S. Santos, N. C. Strøm, P. A. Tsantaki, M. Udry, S. |
| author |
Demangeon, O. D. S. |
| author_facet |
Demangeon, O. D. S. Dalal, S. Hébrard, G. Nsamba, B. Kiefer, F. Camacho, J.D. Sahlmann, J. Arnold, L. Astudillo Defru, Nicola Bonfils, X. Boisse, I. Bouchy, F. Bourrier, V. Campante, T. Delfosse, X. Deleuil, M. Diaz, Rodrigo Fernando Faria, J. Forveille, T. Hara, N. Heidari, N. Hobson, M.J. Lopez, T. Moutou, C. Rey, J. Santerne, A. Sousa, S. Santos, N. C. Strøm, P. A. Tsantaki, M. Udry, S. |
| author_role |
author |
| author2 |
Dalal, S. Hébrard, G. Nsamba, B. Kiefer, F. Camacho, J.D. Sahlmann, J. Arnold, L. Astudillo Defru, Nicola Bonfils, X. Boisse, I. Bouchy, F. Bourrier, V. Campante, T. Delfosse, X. Deleuil, M. Diaz, Rodrigo Fernando Faria, J. Forveille, T. Hara, N. Heidari, N. Hobson, M.J. Lopez, T. Moutou, C. Rey, J. Santerne, A. Sousa, S. Santos, N. C. Strøm, P. A. Tsantaki, M. Udry, S. |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
PLANETS AND SATELLITES: DETECTION TECHNIQUES: RADIAL VELOCITIES |
| topic |
PLANETS AND SATELLITES: DETECTION TECHNIQUES: RADIAL VELOCITIES |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Context. Due to their low transit probability, the long-period planets are, as a population, only partially probed by transit surveys. Radial velocity surveys thus have a key role to play, in particular for giant planets. Cold Jupiters induce a typical radial velocity semi-amplitude of 10 m s-1, which is well within the reach of multiple instruments that have now been in operation for more than a decade. Aims. We take advantage of the ongoing radial velocity survey with the » SOPHIE high-resolution spectrograph, which continues the search started by its predecessor » ELODIE to further characterize the cold Jupiter population. Methods. Analyzing the radial velocity data from six bright solar-like stars taken over a period of up to 15 yr, we attempt the detection and confirmation of Keplerian signals. Results. We announce the discovery of six planets, one per system, with minimum masses in the range 4.8-8.3 Mjup and orbital periods between 200 days and 10 yr. The data do not provide enough evidence to support the presence of additional planets in any of these systems. The analysis of stellar activity indicators confirms the planetary nature of the detected signals. Conclusions. These six planets belong to the cold and massive Jupiter population, and four of them populate its eccentric tail. In this respect, HD 80869 b stands out as having one of the most eccentric orbits, with an eccentricity of 0.862-0.018+0.028. These planets can thus help to better constrain the migration and evolution processes at play in the gas giant population. Furthermore, recent works presenting the correlation between small planets and cold Jupiters indicate that these systems are good candidates to search for small inner planets. Fil: Demangeon, O. D. S.. Universidad de Porto; Portugal Fil: Dalal, S.. Institut d'Astrophysique de Paris; Francia Fil: Hébrard, G.. Institut d'Astrophysique de Paris; Francia. Université d’Aix-Marseille; Francia Fil: Nsamba, B.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania. Mbarara University of Science and Technology; Uganda. Universidad de Porto; Portugal Fil: Kiefer, F.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia. Institut d'Astrophysique de Paris; Francia. Sorbonne University; Francia Fil: Camacho, J.D.. Universidad de Porto; Portugal Fil: Sahlmann, J.. European Space Astronomy Centre; España Fil: Arnold, L.. Université d’Aix-Marseille; Francia Fil: Astudillo Defru, Nicola. Universidad Católica de la Santísima Concepción; Chile Fil: Bonfils, X.. Universite Grenoble Alpes; Francia Fil: Boisse, I.. Université d’Aix-Marseille; Francia Fil: Bouchy, F.. Universidad de Ginebra; Suiza Fil: Bourrier, V.. Universidad de Ginebra; Suiza Fil: Campante, T.. Universidad de Porto; Portugal Fil: Delfosse, X.. Universite Grenoble Alpes; Francia Fil: Deleuil, M.. Université d’Aix-Marseille; Francia Fil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Ciencias Físicas. - Universidad Nacional de San Martín. Instituto de Ciencias Físicas; Argentina. Universidad Nacional de San Martín. Escuela de Política y Gobierno; Argentina Fil: Faria, J.. Universidad de Porto; Portugal Fil: Forveille, T.. Universite Grenoble Alpes; Francia Fil: Hara, N.. Universidad de Ginebra; Suiza Fil: Heidari, N.. Université Nice Sophia Antipolis. Laboratoire Joseph-louis Lagrange; Francia. Shahid Beheshti University; Irán. Université d’Aix-Marseille; Francia Fil: Hobson, M.J.. Instituto Milenio de Astrofísica; Chile. Pontificia Universidad Católica de Chile; Chile Fil: Lopez, T.. Université d’Aix-Marseille; Francia Fil: Moutou, C.. Universite de Toulose - Le Mirail; Francia Fil: Rey, J.. Carnegie Institution of Washington. Las Campanas Observatory; Chile Fil: Santerne, A.. Université d’Aix-Marseille; Francia Fil: Sousa, S.. Universidad de Porto; Portugal Fil: Santos, N. C.. Universidad de Porto; Portugal Fil: Strøm, P. A.. Sorbonne University; Francia. University of Warwick; Reino Unido Fil: Tsantaki, M.. Osservatorio Astrofisico Di Arcetri; Italia. Universidad de Porto; Portugal Fil: Udry, S.. Universidad de Ginebra; Suiza |
| description |
Context. Due to their low transit probability, the long-period planets are, as a population, only partially probed by transit surveys. Radial velocity surveys thus have a key role to play, in particular for giant planets. Cold Jupiters induce a typical radial velocity semi-amplitude of 10 m s-1, which is well within the reach of multiple instruments that have now been in operation for more than a decade. Aims. We take advantage of the ongoing radial velocity survey with the » SOPHIE high-resolution spectrograph, which continues the search started by its predecessor » ELODIE to further characterize the cold Jupiter population. Methods. Analyzing the radial velocity data from six bright solar-like stars taken over a period of up to 15 yr, we attempt the detection and confirmation of Keplerian signals. Results. We announce the discovery of six planets, one per system, with minimum masses in the range 4.8-8.3 Mjup and orbital periods between 200 days and 10 yr. The data do not provide enough evidence to support the presence of additional planets in any of these systems. The analysis of stellar activity indicators confirms the planetary nature of the detected signals. Conclusions. These six planets belong to the cold and massive Jupiter population, and four of them populate its eccentric tail. In this respect, HD 80869 b stands out as having one of the most eccentric orbits, with an eccentricity of 0.862-0.018+0.028. These planets can thus help to better constrain the migration and evolution processes at play in the gas giant population. Furthermore, recent works presenting the correlation between small planets and cold Jupiters indicate that these systems are good candidates to search for small inner planets. |
| publishDate |
2021 |
| dc.date.none.fl_str_mv |
2021-09-10 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/154526 Demangeon, O. D. S.; Dalal, S.; Hébrard, G.; Nsamba, B.; Kiefer, F.; et al.; The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits; EDP Sciences; Astronomy and Astrophysics; 653; A78; 10-9-2021; 1-24 0004-6361 1432-0746 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/154526 |
| identifier_str_mv |
Demangeon, O. D. S.; Dalal, S.; Hébrard, G.; Nsamba, B.; Kiefer, F.; et al.; The SOPHIE search for northern extrasolar planets: XVIII. Six new cold Jupiters, including one of the most eccentric exoplanet orbits; EDP Sciences; Astronomy and Astrophysics; 653; A78; 10-9-2021; 1-24 0004-6361 1432-0746 CONICET Digital CONICET |
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eng |
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eng |
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EDP Sciences |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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