A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N

Autores
König, P. C.; Damasso, M.; Hébrard, G.; Naponiello, L.; Cortés Zuleta, P.; Biazzo, K.; Santos, N. C.; Bonomo, A. S.; Lecavelier des Étangs, A.; Zeng, L.; Hoyer, S.; Sozzetti, A.; Affer, L.; Almenara, J. M.; Benatti, S.; Bieryla, A.; Boisse, I.; Bonfils, X.; Boschin, W.; Carmona, A.; Claudi, R.; Collins, K. A.; Dalal, S.; Deleuil, M.; Diaz, Rodrigo Fernando; Stognone, R. G.; Strøm, P. A.; Vanderspek, R.; Winn, J.; Wittrock, J.
Año de publicación
2022
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We report the discovery and characterization of the transiting extrasolar planet TOI-1710 b. It was first identified as a promising candidate by the Transiting Exoplanet Survey Satellite. Its planetary nature was then established with SOPHIE and HARPS-N spectroscopic observations via the radial-velocity method. The stellar parameters for the host star are derived from the spectra and a joint Markov chain Monte-Carlo adjustment of the spectral energy distribution and evolutionary tracks of TOI-1710. A joint MCMC analysis of the TESS light curve and the radial-velocity evolution allows us to determine the planetary system properties. From our analysis, TOI-1710 b is found to be a massive warm super-Neptune (Mp = 28.3 ± 4.7 M⊕ and Rp = 5.34 ± 0.11 R⊕) orbiting a G5V dwarf star (Teff = 5665 ± 55 K) on a nearly circular 24.3-day orbit (e = 0.16 ± 0.08). The orbital period of this planet is close to the estimated rotation period of its host star Prot = 22.5 ± 2.0 days and it has a low Keplerian semi-amplitude K = 6.4 ± 1.0 m s−1; we thus performed additional analyses to show the robustness of the retrieved planetary parameters. With a low bulk density of 1.03 ± 0.23 g cm−3 and orbiting a bright host star (J = 8.3, V = 9.6), TOI-1710 b is one of the best targets in this mass-radius range (near the Neptunian desert) for atmospheric characterization via transmission spectroscopy, a key measurement in constraining planet formation and evolutionary models of sub-Jovian planets.
Fil: König, P. C.. Sorbonne University; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Damasso, M.. Istituto Nazionale di Astrofisica; Italia
Fil: Hébrard, G.. Sorbonne University; Francia. Université d’Aix-Marseille; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Naponiello, L.. Universita Tor Vergata; Italia. University of Florence; Italia
Fil: Cortés Zuleta, P.. Université d’Aix-Marseille; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Biazzo, K.. Istituto Nazionale di Astrofisica; Italia
Fil: Santos, N. C.. Universidad de Porto; Portugal
Fil: Bonomo, A. S.. Istituto Nazionale di Astrofisica; Italia
Fil: Lecavelier des Étangs, A.. Centre National de la Recherche Scientifique; Francia. Sorbonne University; Francia
Fil: Zeng, L.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Harvard University; Estados Unidos
Fil: Hoyer, S.. Aix-Marseille Université; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Sozzetti, A.. Istituto Nazionale di Astrofisica; Italia
Fil: Affer, L.. Istituto Nazionale di Astrofisica; Italia
Fil: Almenara, J. M.. Universite Grenoble Alpes; Francia
Fil: Benatti, S.. Istituto Nazionale di Astrofisica; Italia
Fil: Bieryla, A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Boisse, I.. Aix-Marseille Université; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Bonfils, X.. Centre National de la Recherche Scientifique; Francia. Universite Grenoble Alpes; Francia
Fil: Boschin, W.. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; España. Fundación Galileo Galilei; Italia
Fil: Carmona, A.. Centre National de la Recherche Scientifique; Francia. Universite Grenoble Alpes; Francia
Fil: Claudi, R.. Osservatorio Astronomico di Padova; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Collins, K. A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Dalal, S.. Centre National de la Recherche Scientifique; Francia. Sorbonne University; Francia
Fil: Deleuil, M.. Osservatorio Astronomico di Padova; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Instituto de Ciencias Fisicas. - Universidad Nacional de San Martin. Instituto de Ciencias Fisicas.; Argentina
Fil: Stognone, R. G.. Università di Torino; Italia
Fil: Strøm, P. A.. University of Princeton; Estados Unidos. Sorbonne University; Francia. University of Warwick; Reino Unido
Fil: Vanderspek, R.. Massachusetts Institute of Technology; Estados Unidos
Fil: Winn, J.. University of Princeton; Estados Unidos
Fil: Wittrock, J.. George Mason University; Estados Unidos
Materia
planetary systems
techniques: photometric
techniques: spectroscopic
techniques: radial velocities
star: activity
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:11336/274361
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/274361
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-NKönig, P. C.Damasso, M.Hébrard, G.Naponiello, L.Cortés Zuleta, P.Biazzo, K.Santos, N. C.Bonomo, A. S.Lecavelier des Étangs, A.Zeng, L.Hoyer, S.Sozzetti, A.Affer, L.Almenara, J. M.Benatti, S.Bieryla, A.Boisse, I.Bonfils, X.Boschin, W.Carmona, A.Claudi, R.Collins, K. A.Dalal, S.Deleuil, M.Diaz, Rodrigo FernandoStognone, R. G.Strøm, P. A.Vanderspek, R.Winn, J.Wittrock, J.planetary systemstechniques: photometrictechniques: spectroscopictechniques: radial velocitiesstar: activityhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We report the discovery and characterization of the transiting extrasolar planet TOI-1710 b. It was first identified as a promising candidate by the Transiting Exoplanet Survey Satellite. Its planetary nature was then established with SOPHIE and HARPS-N spectroscopic observations via the radial-velocity method. The stellar parameters for the host star are derived from the spectra and a joint Markov chain Monte-Carlo adjustment of the spectral energy distribution and evolutionary tracks of TOI-1710. A joint MCMC analysis of the TESS light curve and the radial-velocity evolution allows us to determine the planetary system properties. From our analysis, TOI-1710 b is found to be a massive warm super-Neptune (Mp = 28.3 ± 4.7 M⊕ and Rp = 5.34 ± 0.11 R⊕) orbiting a G5V dwarf star (Teff = 5665 ± 55 K) on a nearly circular 24.3-day orbit (e = 0.16 ± 0.08). The orbital period of this planet is close to the estimated rotation period of its host star Prot = 22.5 ± 2.0 days and it has a low Keplerian semi-amplitude K = 6.4 ± 1.0 m s−1; we thus performed additional analyses to show the robustness of the retrieved planetary parameters. With a low bulk density of 1.03 ± 0.23 g cm−3 and orbiting a bright host star (J = 8.3, V = 9.6), TOI-1710 b is one of the best targets in this mass-radius range (near the Neptunian desert) for atmospheric characterization via transmission spectroscopy, a key measurement in constraining planet formation and evolutionary models of sub-Jovian planets.Fil: König, P. C.. Sorbonne University; Francia. Centre National de la Recherche Scientifique; FranciaFil: Damasso, M.. Istituto Nazionale di Astrofisica; ItaliaFil: Hébrard, G.. Sorbonne University; Francia. Université d’Aix-Marseille; Francia. Centre National de la Recherche Scientifique; FranciaFil: Naponiello, L.. Universita Tor Vergata; Italia. University of Florence; ItaliaFil: Cortés Zuleta, P.. Université d’Aix-Marseille; Francia. Centre National de la Recherche Scientifique; FranciaFil: Biazzo, K.. Istituto Nazionale di Astrofisica; ItaliaFil: Santos, N. C.. Universidad de Porto; PortugalFil: Bonomo, A. S.. Istituto Nazionale di Astrofisica; ItaliaFil: Lecavelier des Étangs, A.. Centre National de la Recherche Scientifique; Francia. Sorbonne University; FranciaFil: Zeng, L.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Harvard University; Estados UnidosFil: Hoyer, S.. Aix-Marseille Université; Francia. Centre National de la Recherche Scientifique; FranciaFil: Sozzetti, A.. Istituto Nazionale di Astrofisica; ItaliaFil: Affer, L.. Istituto Nazionale di Astrofisica; ItaliaFil: Almenara, J. M.. Universite Grenoble Alpes; FranciaFil: Benatti, S.. Istituto Nazionale di Astrofisica; ItaliaFil: Bieryla, A.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Boisse, I.. Aix-Marseille Université; Francia. Centre National de la Recherche Scientifique; FranciaFil: Bonfils, X.. Centre National de la Recherche Scientifique; Francia. Universite Grenoble Alpes; FranciaFil: Boschin, W.. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; España. Fundación Galileo Galilei; ItaliaFil: Carmona, A.. Centre National de la Recherche Scientifique; Francia. Universite Grenoble Alpes; FranciaFil: Claudi, R.. Osservatorio Astronomico di Padova; Italia. Istituto Nazionale di Astrofisica; ItaliaFil: Collins, K. A.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Dalal, S.. Centre National de la Recherche Scientifique; Francia. Sorbonne University; FranciaFil: Deleuil, M.. Osservatorio Astronomico di Padova; Italia. Istituto Nazionale di Astrofisica; ItaliaFil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Instituto de Ciencias Fisicas. - Universidad Nacional de San Martin. Instituto de Ciencias Fisicas.; ArgentinaFil: Stognone, R. G.. Università di Torino; ItaliaFil: Strøm, P. A.. University of Princeton; Estados Unidos. Sorbonne University; Francia. University of Warwick; Reino UnidoFil: Vanderspek, R.. Massachusetts Institute of Technology; Estados UnidosFil: Winn, J.. University of Princeton; Estados UnidosFil: Wittrock, J.. George Mason University; Estados UnidosEDP Sciences2022-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/274361König, P. C.; Damasso, M.; Hébrard, G.; Naponiello, L.; Cortés Zuleta, P.; et al.; A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N; EDP Sciences; Astronomy and Astrophysics; 666; A183; 10-2022; 1-180004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/10.1051/0004-6361/202143002info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202143002info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-11-12T09:45:43Zoai:ri.conicet.gov.ar:11336/274361instacron: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:34982025-11-12 09:45:43.916CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
title A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
spellingShingle A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
König, P. C.
planetary systems
techniques: photometric
techniques: spectroscopic
techniques: radial velocities
star: activity
title_short A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
title_full A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
title_fullStr A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
title_full_unstemmed A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
title_sort A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
dc.creator.none.fl_str_mv König, P. C.
Damasso, M.
Hébrard, G.
Naponiello, L.
Cortés Zuleta, P.
Biazzo, K.
Santos, N. C.
Bonomo, A. S.
Lecavelier des Étangs, A.
Zeng, L.
Hoyer, S.
Sozzetti, A.
Affer, L.
Almenara, J. M.
Benatti, S.
Bieryla, A.
Boisse, I.
Bonfils, X.
Boschin, W.
Carmona, A.
Claudi, R.
Collins, K. A.
Dalal, S.
Deleuil, M.
Diaz, Rodrigo Fernando
Stognone, R. G.
Strøm, P. A.
Vanderspek, R.
Winn, J.
Wittrock, J.
author König, P. C.
author_facet König, P. C.
Damasso, M.
Hébrard, G.
Naponiello, L.
Cortés Zuleta, P.
Biazzo, K.
Santos, N. C.
Bonomo, A. S.
Lecavelier des Étangs, A.
Zeng, L.
Hoyer, S.
Sozzetti, A.
Affer, L.
Almenara, J. M.
Benatti, S.
Bieryla, A.
Boisse, I.
Bonfils, X.
Boschin, W.
Carmona, A.
Claudi, R.
Collins, K. A.
Dalal, S.
Deleuil, M.
Diaz, Rodrigo Fernando
Stognone, R. G.
Strøm, P. A.
Vanderspek, R.
Winn, J.
Wittrock, J.
author_role author
author2 Damasso, M.
Hébrard, G.
Naponiello, L.
Cortés Zuleta, P.
Biazzo, K.
Santos, N. C.
Bonomo, A. S.
Lecavelier des Étangs, A.
Zeng, L.
Hoyer, S.
Sozzetti, A.
Affer, L.
Almenara, J. M.
Benatti, S.
Bieryla, A.
Boisse, I.
Bonfils, X.
Boschin, W.
Carmona, A.
Claudi, R.
Collins, K. A.
Dalal, S.
Deleuil, M.
Diaz, Rodrigo Fernando
Stognone, R. G.
Strøm, P. A.
Vanderspek, R.
Winn, J.
Wittrock, J.
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
dc.subject.none.fl_str_mv planetary systems
techniques: photometric
techniques: spectroscopic
techniques: radial velocities
star: activity
topic planetary systems
techniques: photometric
techniques: spectroscopic
techniques: radial velocities
star: activity
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We report the discovery and characterization of the transiting extrasolar planet TOI-1710 b. It was first identified as a promising candidate by the Transiting Exoplanet Survey Satellite. Its planetary nature was then established with SOPHIE and HARPS-N spectroscopic observations via the radial-velocity method. The stellar parameters for the host star are derived from the spectra and a joint Markov chain Monte-Carlo adjustment of the spectral energy distribution and evolutionary tracks of TOI-1710. A joint MCMC analysis of the TESS light curve and the radial-velocity evolution allows us to determine the planetary system properties. From our analysis, TOI-1710 b is found to be a massive warm super-Neptune (Mp = 28.3 ± 4.7 M⊕ and Rp = 5.34 ± 0.11 R⊕) orbiting a G5V dwarf star (Teff = 5665 ± 55 K) on a nearly circular 24.3-day orbit (e = 0.16 ± 0.08). The orbital period of this planet is close to the estimated rotation period of its host star Prot = 22.5 ± 2.0 days and it has a low Keplerian semi-amplitude K = 6.4 ± 1.0 m s−1; we thus performed additional analyses to show the robustness of the retrieved planetary parameters. With a low bulk density of 1.03 ± 0.23 g cm−3 and orbiting a bright host star (J = 8.3, V = 9.6), TOI-1710 b is one of the best targets in this mass-radius range (near the Neptunian desert) for atmospheric characterization via transmission spectroscopy, a key measurement in constraining planet formation and evolutionary models of sub-Jovian planets.
Fil: König, P. C.. Sorbonne University; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Damasso, M.. Istituto Nazionale di Astrofisica; Italia
Fil: Hébrard, G.. Sorbonne University; Francia. Université d’Aix-Marseille; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Naponiello, L.. Universita Tor Vergata; Italia. University of Florence; Italia
Fil: Cortés Zuleta, P.. Université d’Aix-Marseille; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Biazzo, K.. Istituto Nazionale di Astrofisica; Italia
Fil: Santos, N. C.. Universidad de Porto; Portugal
Fil: Bonomo, A. S.. Istituto Nazionale di Astrofisica; Italia
Fil: Lecavelier des Étangs, A.. Centre National de la Recherche Scientifique; Francia. Sorbonne University; Francia
Fil: Zeng, L.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Harvard University; Estados Unidos
Fil: Hoyer, S.. Aix-Marseille Université; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Sozzetti, A.. Istituto Nazionale di Astrofisica; Italia
Fil: Affer, L.. Istituto Nazionale di Astrofisica; Italia
Fil: Almenara, J. M.. Universite Grenoble Alpes; Francia
Fil: Benatti, S.. Istituto Nazionale di Astrofisica; Italia
Fil: Bieryla, A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Boisse, I.. Aix-Marseille Université; Francia. Centre National de la Recherche Scientifique; Francia
Fil: Bonfils, X.. Centre National de la Recherche Scientifique; Francia. Universite Grenoble Alpes; Francia
Fil: Boschin, W.. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; España. Fundación Galileo Galilei; Italia
Fil: Carmona, A.. Centre National de la Recherche Scientifique; Francia. Universite Grenoble Alpes; Francia
Fil: Claudi, R.. Osservatorio Astronomico di Padova; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Collins, K. A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Dalal, S.. Centre National de la Recherche Scientifique; Francia. Sorbonne University; Francia
Fil: Deleuil, M.. Osservatorio Astronomico di Padova; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Instituto de Ciencias Fisicas. - Universidad Nacional de San Martin. Instituto de Ciencias Fisicas.; Argentina
Fil: Stognone, R. G.. Università di Torino; Italia
Fil: Strøm, P. A.. University of Princeton; Estados Unidos. Sorbonne University; Francia. University of Warwick; Reino Unido
Fil: Vanderspek, R.. Massachusetts Institute of Technology; Estados Unidos
Fil: Winn, J.. University of Princeton; Estados Unidos
Fil: Wittrock, J.. George Mason University; Estados Unidos
description We report the discovery and characterization of the transiting extrasolar planet TOI-1710 b. It was first identified as a promising candidate by the Transiting Exoplanet Survey Satellite. Its planetary nature was then established with SOPHIE and HARPS-N spectroscopic observations via the radial-velocity method. The stellar parameters for the host star are derived from the spectra and a joint Markov chain Monte-Carlo adjustment of the spectral energy distribution and evolutionary tracks of TOI-1710. A joint MCMC analysis of the TESS light curve and the radial-velocity evolution allows us to determine the planetary system properties. From our analysis, TOI-1710 b is found to be a massive warm super-Neptune (Mp = 28.3 ± 4.7 M⊕ and Rp = 5.34 ± 0.11 R⊕) orbiting a G5V dwarf star (Teff = 5665 ± 55 K) on a nearly circular 24.3-day orbit (e = 0.16 ± 0.08). The orbital period of this planet is close to the estimated rotation period of its host star Prot = 22.5 ± 2.0 days and it has a low Keplerian semi-amplitude K = 6.4 ± 1.0 m s−1; we thus performed additional analyses to show the robustness of the retrieved planetary parameters. With a low bulk density of 1.03 ± 0.23 g cm−3 and orbiting a bright host star (J = 8.3, V = 9.6), TOI-1710 b is one of the best targets in this mass-radius range (near the Neptunian desert) for atmospheric characterization via transmission spectroscopy, a key measurement in constraining planet formation and evolutionary models of sub-Jovian planets.
publishDate 2022
dc.date.none.fl_str_mv 2022-10
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/11336/274361
König, P. C.; Damasso, M.; Hébrard, G.; Naponiello, L.; Cortés Zuleta, P.; et al.; A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N; EDP Sciences; Astronomy and Astrophysics; 666; A183; 10-2022; 1-18
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/274361
identifier_str_mv König, P. C.; Damasso, M.; Hébrard, G.; Naponiello, L.; Cortés Zuleta, P.; et al.; A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N; EDP Sciences; Astronomy and Astrophysics; 666; A183; 10-2022; 1-18
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/url/https://www.aanda.org/10.1051/0004-6361/202143002
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202143002
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
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score 12.976206

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