Dataciencia

Colección SciELO Chile

A SOPHIE RV search for giant planets around young nearby stars (YNS): A combination with the HARPS YNS survey

Indexado

WoS	WOS:000660894300001
Scopus	SCOPUS_ID:85107568967

DOI

10.1051/0004-6361/202039672

Año

2021

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Results. We report one new trend compatible with a planetary companion on HD 109647. We also report HD 105693 and HD 112097 as binaries, and we confirm the binarity of HD 2454, HD 13531, HD 17250 A, HD 28945, HD 39587, HD 131156, HD 142229, HD 186704 A, and HD 195943. We constrained for the first time the orbital parameters of HD 195943 B. We refute the HD 13507 single brown dwarf (BD) companion solution and propose a double BD companion solution. Two GPs were previously reported from this survey in the HD 113337 system. Based on our sample of 120 young stars, we obtain a GP occurrence rate of 1 +2:2 0:3 % for periods lower than 1000 days, and we obtain an upper limit on BD occurrence rate of 0:9+2 0:9% in the same period range. We report a possible lack of close ( P 2 [1; 1000] days) GPs around young FK stars compared to their older counterparts, with a confidence level of 90%.

Revista

Revista	ISSN
Astronomy & Astrophysics	0004-6361

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Grandjean, Antoine	Hombre	Univ Grenoble Alpes - Francia Universite Grenoble Alpes - Francia
2	Lagrange, A. -m.	Mujer	Univ Grenoble Alpes - Francia UNIV PARIS - Francia IMCCE Observ Paris - Francia Universite Grenoble Alpes - Francia L'Observatoire de Paris - Francia
3	Meunier, Nadege	-	Univ Grenoble Alpes - Francia Universite Grenoble Alpes - Francia
4	Rubini, Pascal	Hombre	Pixyl - Francia
5	Desidera, S.	Hombre	Istituto Nazionale di Astrofisica - Italia Osservatorio Astronomico di Padova - Italia INAF Osservatorio Astron Padova - Italia
6	Galland, Franck	Hombre	Univ Grenoble Alpes - Francia Universite Grenoble Alpes - Francia
7	Borgniet, Simon	Hombre	CNRS Lesia UMR8109 - Francia L'Observatoire de Paris - Francia
8	Zicher, N.	-	Oxford Astrophys - Reino Unido University of Oxford - Reino Unido
9	Messina, Sergio	Hombre	Istituto Nazionale di Astrofisica - Italia Osservatorio Astrofisico di Catania - Italia INAF Osservatorio Astrofis Catania - Italia
10	Chauvin, Gael	Hombre	Univ Grenoble Alpes - Francia Universite Grenoble Alpes - Francia
11	Sterzik, Michael	Hombre	ESO - Alemania Observatorio Europeo Austral - Alemania European Southern Observ - Alemania
12	Pantoja, B.	-	Universidad de Chile - Chile

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Financiamiento

Fuente
Agence Nationale de la Recherche
French CNRS
INAF/Frontiera through the "Progetti Premiali" funding scheme of the Italian Ministry of Education, University, and Research
Ministero dell’Istruzione, dell’Università e della Ricerca
Labex
Centre National de la Recherche Scientifique
European Southern Observatory
Istituto Nazionale di Astrofisica
Labex OSUG
"European Southern Observatory"
'European Southern Observatory'
The European Southern Observatory
Observatoire de Haute Provence
Agence Nationale de la Recherche (ANR grant GIPSE)
FRONTIERA

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Agradecimientos

Agradecimiento
We acknowledge support from the French CNRS and from the Agence Nationale de la Recherche (ANR grant GIPSE ANR-14-CE33-0018). This work has been supported by a grant from Labex OSUG@2020 (Investissements d'avenir - ANR10 LABX56). These results have made use of the SIMBAD database, operated at the CDS, Strasbourg, France. ESO SD acknowledges the support by INAF/Frontiera through the "Progetti Premiali" funding scheme of the Italian Ministry of Education, University, and Research. Based on observations collected at the European Southern Observatory under ESO programme(s) 060.A-9036(A), 072.C-0488(E), 072.C-0636(A), 072.C-0636(B), 073.C-0733(A), 073.C-0733(C), 073.C-0733(D), 073.C-0733(E), 074.C-0037(A), 074.C-0364(A), 075.C-0202(A), 075.C-0234(A), 075.C-0234(B), 075.C-0689(A), 075.C-0689(B), 076.C-0010(A), 076.C-0073(A), 076.C-0279(A), 076.C-0279(B), 076.C-0279(C), 077.C-0012(A), 077.C-0295(A), 077.C-0295(B), 077.C-0295(C), 077.C-0295(D), 078.C-0209(A), 078.C-0209(B), 078.C-0751(A), 078.C-0751(B), 079.C-0170(A), 079.C-0170(B), 079.C-0657(C), 080.C-0032(A), 080.C-0032(B), 080.C-0664(A), 080.C-0712(A), 081.C-0034(B), 081.C-0802(C), 082.C-0308(A), 082.C-0357(A), 082.C-0412(A), 082.C-0427(A), 082.C-0427(C), 082.C-0718(B), 083.C-0794(A), 083.C-0794(B), 083.C-0794(C), 083.C-0794(D), 084.C-1039(A), 085.C-0019(A), 087.C-0831(A), 089.C-0732(A), 089.C-0739(A), 090.C-0421(A), 091.C-0034(A), 094.C-0946(A), 098.C-0739(A), 099.C-0205(A), 0104.C-0418(A), 1101.C-0557(A), 183.C-0437(A), 183.C-0972(A), 184.C-0815(A), 184.C-0815(B), 184.C-0815(C), 184.C-0815(E), 184.C-0815(F), 191.C-0873(A), 192.C-0224(B), 192.C-0224(C), 192.C-0224(G), 192.C-0224(H). Based on observations collected at the Observatoire de Haute Provence under the programme(s) 06B.PNP.CONS, 07A.PNP.CONS, 07B.PNP.CONS, 08A.PNP.CONS, 13A.PNP.DELF, 13A.PNP.LAGR, 14A.PNP.LAGR.
Acknowledgements. We acknowledge support from the French CNRS and from the Agence Nationale de la Recherche (ANR grant GIPSE ANR-14-CE33-0018). This work has been supported by a grant from Labex OSUG@2020 (Investisse-ments d’avenir – ANR10 LABX56). These results have made use of the SIMBAD database, operated at the CDS, Strasbourg, France. ESO SD acknowledges the support by INAF/Frontiera through the “Progetti Premiali” funding scheme of the Italian Ministry of Education, University, and Research. Based on observations collected at the European Southern Observatory under ESO programme(s) 060.A-9036(A), 072.C-0488(E), 072.C-0636(A), 072.C-0636(B), 073.C-0733(A), 073.C-0733(C), 073.C-0733(D), 073.C-0733(E), 074.C-0037(A), 074.C-0364(A), 075.C-0202(A), 075.C-0234(A), 075.C-0234(B), 075.C-0689(A), 075.C-0689(B), 076.C-0010(A), 076.C-0073(A), 076.C-0279(A), 076.C-0279(B), 076.C-0279(C), 077.C-0012(A), 077.C-0295(A), 077.C-0295(B), 077.C-0295(C), 077.C-0295(D), 078.C-0209(A), 078.C-0209(B), 078.C-0751(A), 078.C-0751(B), 079.C-0170(A), 079.C-0170(B), 079.C-0657(C), 080.C-0032(A), 080.C-0032(B), 080.C-0664(A), 080.C-0712(A), 081.C-0034(B), 081.C-0802(C), 082.C-0308(A), 082.C-0357(A), 082.C-0412(A), 082.C-0427(A), 082.C-0427(C), 082.C-0718(B), 083.C-0794(A), 083.C-0794(B), 083.C-0794(C), 083.C-0794(D), 084.C-1039(A), 085.C-0019(A), 087.C-0831(A), 089.C-0732(A), 089.C-0739(A), 090.C-0421(A), 091.C-0034(A), 094.C-0946(A), 098.C-0739(A), 099.C-0205(A), 0104.C-0418(A), 1101.C-0557(A), 183.C-0437(A), 183.C-0972(A), 184.C-0815(A), 184.C-0815(B), 184.C-0815(C), 184.C-0815(E), 184.C-0815(F), 191.C-0873(A), 192.C-0224(B), 192.C-0224(C), 192.C-0224(G), 192.C-0224(H). Based on observations collected at the Observatoire de Haute Provence under the programme(s) 06B.PNP.CONS, 07A.PNP.CONS, 07B.PNP.CONS, 08A.PNP.CONS, 13A.PNP.DELF, 13A.PNP.LAGR, 14A.PNP.LAGR.

Agradecimiento

We acknowledge support from the French CNRS and from the Agence Nationale de la Recherche (ANR grant GIPSE ANR-14-CE33-0018). This work has been supported by a grant from Labex OSUG@2020 (Investissements d'avenir - ANR10 LABX56). These results have made use of the SIMBAD database, operated at the CDS, Strasbourg, France. ESO SD acknowledges the support by INAF/Frontiera through the "Progetti Premiali" funding scheme of the Italian Ministry of Education, University, and Research. Based on observations collected at the European Southern Observatory under ESO programme(s) 060.A-9036(A), 072.C-0488(E), 072.C-0636(A), 072.C-0636(B), 073.C-0733(A), 073.C-0733(C), 073.C-0733(D), 073.C-0733(E), 074.C-0037(A), 074.C-0364(A), 075.C-0202(A), 075.C-0234(A), 075.C-0234(B), 075.C-0689(A), 075.C-0689(B), 076.C-0010(A), 076.C-0073(A), 076.C-0279(A), 076.C-0279(B), 076.C-0279(C), 077.C-0012(A), 077.C-0295(A), 077.C-0295(B), 077.C-0295(C), 077.C-0295(D), 078.C-0209(A), 078.C-0209(B), 078.C-0751(A), 078.C-0751(B), 079.C-0170(A), 079.C-0170(B), 079.C-0657(C), 080.C-0032(A), 080.C-0032(B), 080.C-0664(A), 080.C-0712(A), 081.C-0034(B), 081.C-0802(C), 082.C-0308(A), 082.C-0357(A), 082.C-0412(A), 082.C-0427(A), 082.C-0427(C), 082.C-0718(B), 083.C-0794(A), 083.C-0794(B), 083.C-0794(C), 083.C-0794(D), 084.C-1039(A), 085.C-0019(A), 087.C-0831(A), 089.C-0732(A), 089.C-0739(A), 090.C-0421(A), 091.C-0034(A), 094.C-0946(A), 098.C-0739(A), 099.C-0205(A), 0104.C-0418(A), 1101.C-0557(A), 183.C-0437(A), 183.C-0972(A), 184.C-0815(A), 184.C-0815(B), 184.C-0815(C), 184.C-0815(E), 184.C-0815(F), 191.C-0873(A), 192.C-0224(B), 192.C-0224(C), 192.C-0224(G), 192.C-0224(H). Based on observations collected at the Observatoire de Haute Provence under the programme(s) 06B.PNP.CONS, 07A.PNP.CONS, 07B.PNP.CONS, 08A.PNP.CONS, 13A.PNP.DELF, 13A.PNP.LAGR, 14A.PNP.LAGR.

Acknowledgements. We acknowledge support from the French CNRS and from the Agence Nationale de la Recherche (ANR grant GIPSE ANR-14-CE33-0018). This work has been supported by a grant from Labex OSUG@2020 (Investisse-ments d’avenir – ANR10 LABX56). These results have made use of the SIMBAD database, operated at the CDS, Strasbourg, France. ESO SD acknowledges the support by INAF/Frontiera through the “Progetti Premiali” funding scheme of the Italian Ministry of Education, University, and Research. Based on observations collected at the European Southern Observatory under ESO programme(s) 060.A-9036(A), 072.C-0488(E), 072.C-0636(A), 072.C-0636(B), 073.C-0733(A), 073.C-0733(C), 073.C-0733(D), 073.C-0733(E), 074.C-0037(A), 074.C-0364(A), 075.C-0202(A), 075.C-0234(A), 075.C-0234(B), 075.C-0689(A), 075.C-0689(B), 076.C-0010(A), 076.C-0073(A), 076.C-0279(A), 076.C-0279(B), 076.C-0279(C), 077.C-0012(A), 077.C-0295(A), 077.C-0295(B), 077.C-0295(C), 077.C-0295(D), 078.C-0209(A), 078.C-0209(B), 078.C-0751(A), 078.C-0751(B), 079.C-0170(A), 079.C-0170(B), 079.C-0657(C), 080.C-0032(A), 080.C-0032(B), 080.C-0664(A), 080.C-0712(A), 081.C-0034(B), 081.C-0802(C), 082.C-0308(A), 082.C-0357(A), 082.C-0412(A), 082.C-0427(A), 082.C-0427(C), 082.C-0718(B), 083.C-0794(A), 083.C-0794(B), 083.C-0794(C), 083.C-0794(D), 084.C-1039(A), 085.C-0019(A), 087.C-0831(A), 089.C-0732(A), 089.C-0739(A), 090.C-0421(A), 091.C-0034(A), 094.C-0946(A), 098.C-0739(A), 099.C-0205(A), 0104.C-0418(A), 1101.C-0557(A), 183.C-0437(A), 183.C-0972(A), 184.C-0815(A), 184.C-0815(B), 184.C-0815(C), 184.C-0815(E), 184.C-0815(F), 191.C-0873(A), 192.C-0224(B), 192.C-0224(C), 192.C-0224(G), 192.C-0224(H). Based on observations collected at the Observatoire de Haute Provence under the programme(s) 06B.PNP.CONS, 07A.PNP.CONS, 07B.PNP.CONS, 08A.PNP.CONS, 13A.PNP.DELF, 13A.PNP.LAGR, 14A.PNP.LAGR.