SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b

Autores
Hébrard, G.; Bonomo, A.S.; Diaz, Rodrigo Fernando; Santerne, A.; Santos, N.C.; Almenara, J.M.; Barros, S.C.C.; Boisse, I.; Bouchy, F.; Bruno, G.; Courcol, B.; Deleuil, M.; Demangeon, O.; Guillot, T.; Montagnier, G.; Moutou, C.; Rey, J.; Wilson, P.A.
Año de publicación
2019
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Whereas thousands of transiting giant exoplanets are known today, only a few are well characterized with long orbital periods. Here we present KOI-3680b, a new planet in this category. First identified by the Kepler team as a promising candidate from the photometry of the Kepler spacecraft, we establish here its planetary nature from the radial velocity follow-up secured over 2 yr with the SOPHIE spectrograph at Observatoire de Haute-Provence, France. The combined analysis of the whole dataset allows us to fully characterize this new planetary system. KOI-3680b has an orbital period of 141.2417 ± 0.0001 days, a mass of 1.93 ± 0.20 MJup, and a radius of 0.99 ± 0.07 RJup. It exhibits a highly eccentric orbit (e = 0.50 ± 0.03) around an early G dwarf. KOI-3680b is the transiting giant planet with the longest period characterized so far around a single star; it offers opportunities to extend studies which were mainly devoted to exoplanets close to their host stars, and to compare both exoplanet populations.
Fil: Hébrard, G.. Centre National de la Recherche Scientifique; Francia
Fil: Bonomo, A.S.. Istituto Nazionale di Astrofisica; Italia
Fil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Santerne, A.. Centre National de la Recherche Scientifique; Francia
Fil: Santos, N.C.. Universidad de Porto; Portugal
Fil: Almenara, J.M.. Centre National de la Recherche Scientifique; Francia
Fil: Barros, S.C.C.. Universidad de Porto; Portugal
Fil: Boisse, I.. Centre National de la Recherche Scientifique; Francia
Fil: Bouchy, F.. Universidad de Ginebra; Suiza
Fil: Bruno, G.. Centre National de la Recherche Scientifique; Francia
Fil: Courcol, B.. Centre National de la Recherche Scientifique; Francia
Fil: Deleuil, M.. Centre National de la Recherche Scientifique; Francia
Fil: Demangeon, O.. Universidad de Porto; Portugal
Fil: Guillot, T.. Centre National de la Recherche Scientifique; Francia
Fil: Montagnier, G.. Centre National de la Recherche Scientifique; Francia
Fil: Moutou, C.. Centre National de la Recherche Scientifique; Francia
Fil: Rey, J.. Universidad de Ginebra; Suiza
Fil: Wilson, P.A.. University of Warwick; Reino Unido
Materia
PLANETARY SYSTEMS
STARS: INDIVIDUAL: KOI-3680
TECHNIQUES: PHOTOMETRIC
TECHNIQUES: RADIAL VELOCITIES
TECHNIQUES: SPECTROSCOPIC
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/150868
Acceder
id CONICETDig_365d5a43ed4072417e6a1eab86a07f7c
oai_identifier_str oai:ri.conicet.gov.ar:11336/150868
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680bHébrard, G.Bonomo, A.S.Diaz, Rodrigo FernandoSanterne, A.Santos, N.C.Almenara, J.M.Barros, S.C.C.Boisse, I.Bouchy, F.Bruno, G.Courcol, B.Deleuil, M.Demangeon, O.Guillot, T.Montagnier, G.Moutou, C.Rey, J.Wilson, P.A.PLANETARY SYSTEMSSTARS: INDIVIDUAL: KOI-3680TECHNIQUES: PHOTOMETRICTECHNIQUES: RADIAL VELOCITIESTECHNIQUES: SPECTROSCOPIChttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Whereas thousands of transiting giant exoplanets are known today, only a few are well characterized with long orbital periods. Here we present KOI-3680b, a new planet in this category. First identified by the Kepler team as a promising candidate from the photometry of the Kepler spacecraft, we establish here its planetary nature from the radial velocity follow-up secured over 2 yr with the SOPHIE spectrograph at Observatoire de Haute-Provence, France. The combined analysis of the whole dataset allows us to fully characterize this new planetary system. KOI-3680b has an orbital period of 141.2417 ± 0.0001 days, a mass of 1.93 ± 0.20 MJup, and a radius of 0.99 ± 0.07 RJup. It exhibits a highly eccentric orbit (e = 0.50 ± 0.03) around an early G dwarf. KOI-3680b is the transiting giant planet with the longest period characterized so far around a single star; it offers opportunities to extend studies which were mainly devoted to exoplanets close to their host stars, and to compare both exoplanet populations.Fil: Hébrard, G.. Centre National de la Recherche Scientifique; FranciaFil: Bonomo, A.S.. Istituto Nazionale di Astrofisica; ItaliaFil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Santerne, A.. Centre National de la Recherche Scientifique; FranciaFil: Santos, N.C.. Universidad de Porto; PortugalFil: Almenara, J.M.. Centre National de la Recherche Scientifique; FranciaFil: Barros, S.C.C.. Universidad de Porto; PortugalFil: Boisse, I.. Centre National de la Recherche Scientifique; FranciaFil: Bouchy, F.. Universidad de Ginebra; SuizaFil: Bruno, G.. Centre National de la Recherche Scientifique; FranciaFil: Courcol, B.. Centre National de la Recherche Scientifique; FranciaFil: Deleuil, M.. Centre National de la Recherche Scientifique; FranciaFil: Demangeon, O.. Universidad de Porto; PortugalFil: Guillot, T.. Centre National de la Recherche Scientifique; FranciaFil: Montagnier, G.. Centre National de la Recherche Scientifique; FranciaFil: Moutou, C.. Centre National de la Recherche Scientifique; FranciaFil: Rey, J.. Universidad de Ginebra; SuizaFil: Wilson, P.A.. University of Warwick; Reino UnidoEDP Sciences2019-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/150868Hébrard, G.; Bonomo, A.S.; Diaz, Rodrigo Fernando; Santerne, A.; Santos, N.C.; et al.; SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b; EDP Sciences; Astronomy and Astrophysics; 623; 3-2019; 1-100004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201834333info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T12:06:22Zoai:ri.conicet.gov.ar:11336/150868instacron: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 12:06:22.398CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b
title SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b
spellingShingle SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b
Hébrard, G.
PLANETARY SYSTEMS
STARS: INDIVIDUAL: KOI-3680
TECHNIQUES: PHOTOMETRIC
TECHNIQUES: RADIAL VELOCITIES
TECHNIQUES: SPECTROSCOPIC
title_short SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b
title_full SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b
title_fullStr SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b
title_full_unstemmed SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b
title_sort SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b
dc.creator.none.fl_str_mv Hébrard, G.
Bonomo, A.S.
Diaz, Rodrigo Fernando
Santerne, A.
Santos, N.C.
Almenara, J.M.
Barros, S.C.C.
Boisse, I.
Bouchy, F.
Bruno, G.
Courcol, B.
Deleuil, M.
Demangeon, O.
Guillot, T.
Montagnier, G.
Moutou, C.
Rey, J.
Wilson, P.A.
author Hébrard, G.
author_facet Hébrard, G.
Bonomo, A.S.
Diaz, Rodrigo Fernando
Santerne, A.
Santos, N.C.
Almenara, J.M.
Barros, S.C.C.
Boisse, I.
Bouchy, F.
Bruno, G.
Courcol, B.
Deleuil, M.
Demangeon, O.
Guillot, T.
Montagnier, G.
Moutou, C.
Rey, J.
Wilson, P.A.
author_role author
author2 Bonomo, A.S.
Diaz, Rodrigo Fernando
Santerne, A.
Santos, N.C.
Almenara, J.M.
Barros, S.C.C.
Boisse, I.
Bouchy, F.
Bruno, G.
Courcol, B.
Deleuil, M.
Demangeon, O.
Guillot, T.
Montagnier, G.
Moutou, C.
Rey, J.
Wilson, P.A.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv PLANETARY SYSTEMS
STARS: INDIVIDUAL: KOI-3680
TECHNIQUES: PHOTOMETRIC
TECHNIQUES: RADIAL VELOCITIES
TECHNIQUES: SPECTROSCOPIC
topic PLANETARY SYSTEMS
STARS: INDIVIDUAL: KOI-3680
TECHNIQUES: PHOTOMETRIC
TECHNIQUES: RADIAL VELOCITIES
TECHNIQUES: SPECTROSCOPIC
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Whereas thousands of transiting giant exoplanets are known today, only a few are well characterized with long orbital periods. Here we present KOI-3680b, a new planet in this category. First identified by the Kepler team as a promising candidate from the photometry of the Kepler spacecraft, we establish here its planetary nature from the radial velocity follow-up secured over 2 yr with the SOPHIE spectrograph at Observatoire de Haute-Provence, France. The combined analysis of the whole dataset allows us to fully characterize this new planetary system. KOI-3680b has an orbital period of 141.2417 ± 0.0001 days, a mass of 1.93 ± 0.20 MJup, and a radius of 0.99 ± 0.07 RJup. It exhibits a highly eccentric orbit (e = 0.50 ± 0.03) around an early G dwarf. KOI-3680b is the transiting giant planet with the longest period characterized so far around a single star; it offers opportunities to extend studies which were mainly devoted to exoplanets close to their host stars, and to compare both exoplanet populations.
Fil: Hébrard, G.. Centre National de la Recherche Scientifique; Francia
Fil: Bonomo, A.S.. Istituto Nazionale di Astrofisica; Italia
Fil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Santerne, A.. Centre National de la Recherche Scientifique; Francia
Fil: Santos, N.C.. Universidad de Porto; Portugal
Fil: Almenara, J.M.. Centre National de la Recherche Scientifique; Francia
Fil: Barros, S.C.C.. Universidad de Porto; Portugal
Fil: Boisse, I.. Centre National de la Recherche Scientifique; Francia
Fil: Bouchy, F.. Universidad de Ginebra; Suiza
Fil: Bruno, G.. Centre National de la Recherche Scientifique; Francia
Fil: Courcol, B.. Centre National de la Recherche Scientifique; Francia
Fil: Deleuil, M.. Centre National de la Recherche Scientifique; Francia
Fil: Demangeon, O.. Universidad de Porto; Portugal
Fil: Guillot, T.. Centre National de la Recherche Scientifique; Francia
Fil: Montagnier, G.. Centre National de la Recherche Scientifique; Francia
Fil: Moutou, C.. Centre National de la Recherche Scientifique; Francia
Fil: Rey, J.. Universidad de Ginebra; Suiza
Fil: Wilson, P.A.. University of Warwick; Reino Unido
description Whereas thousands of transiting giant exoplanets are known today, only a few are well characterized with long orbital periods. Here we present KOI-3680b, a new planet in this category. First identified by the Kepler team as a promising candidate from the photometry of the Kepler spacecraft, we establish here its planetary nature from the radial velocity follow-up secured over 2 yr with the SOPHIE spectrograph at Observatoire de Haute-Provence, France. The combined analysis of the whole dataset allows us to fully characterize this new planetary system. KOI-3680b has an orbital period of 141.2417 ± 0.0001 days, a mass of 1.93 ± 0.20 MJup, and a radius of 0.99 ± 0.07 RJup. It exhibits a highly eccentric orbit (e = 0.50 ± 0.03) around an early G dwarf. KOI-3680b is the transiting giant planet with the longest period characterized so far around a single star; it offers opportunities to extend studies which were mainly devoted to exoplanets close to their host stars, and to compare both exoplanet populations.
publishDate 2019
dc.date.none.fl_str_mv 2019-03
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/150868
Hébrard, G.; Bonomo, A.S.; Diaz, Rodrigo Fernando; Santerne, A.; Santos, N.C.; et al.; SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b; EDP Sciences; Astronomy and Astrophysics; 623; 3-2019; 1-10
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/150868
identifier_str_mv Hébrard, G.; Bonomo, A.S.; Diaz, Rodrigo Fernando; Santerne, A.; Santos, N.C.; et al.; SOPHIE velocimetry of Kepler transit candidates: XIX. the transiting temperate giant planet KOI-3680b; EDP Sciences; Astronomy and Astrophysics; 623; 3-2019; 1-10
0004-6361
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201834333
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1846782420335984640
score 12.982451

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