Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2

Autores
Marchesini, Ezequiel Joaquín; Reynaldi, María Victoria; Vieyro, Florencia Laura; Saponara, Juliana; Andruchow, Ileana; Lopez, I. E.; Benaglia, Paula; Cellone, Sergio Aldo; Masetti, Nicola; Massaro, F.; Peña Herazo, H. A.; Chavushyan, Vahram; Combi, Jorge Ariel; Acosta Pulido, J. A.; Agis Gonzalez, B.; Castro Segura, N.
Año de publicación
2022
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Context. The gamma-ray emitting source WISE J141046.00+740511.2 has been associated with a Fermi-LAT detection by crossmatching with Swift/XRT data. It has shown all the canonical observational characteristics of a BL Lac source, including a power-law, featureless optical spectrum. However, it was only recently detected at radio frequencies and its radio flux is significantly low. Aims. Given that a radio detection is fundamental to associate lower-energy counterparts to Fermi-LAT sources, we aim to unambiguously classify this source by performing a multiwavelength analysis based on contemporaneous data. Methods. By using multifrequency observations at the Jansky Very Large Array, Giant Metrewave Radio Telescope, Gran Telescopio Canarias, Gemini, William Herschel Telescope and Liverpool observatories, together with Fermi-LAT and Swift data, we carried out two kinds of analyses. On one hand, we studied several known parameters that account for the radio loudness or weakness characterization and their application to blazars (in general) and to our source (in particular). And, on the other hand, we built and analyzed the observed spectral energy distribution (SED) of this source to try to explain its peculiar characteristics. Results. The multiwavelength analysis indicates that WISE J141046.00+740511.2 is a blazar of the high-frequency peaked (HBL) type that emits highly polarized light and that is likely located at a low redshift. In addition, the one-zone model parameters that best fit its SED are those of an extreme HBL (EHBL); this blazar type has been extensively predicted in theory to be lacking in the radio emission that is otherwise typical of canonical gamma-ray blazars. Conclusions. We confirm that WISE J141046.00+740511.2 is indeed a highly polarized BL Lac of the HBL type. Further studies will be conducted to explain the atypical low radio flux detected for this source.
Fil: Marchesini, Ezequiel Joaquín. Istituto Di Astrofisica Spaziale E Fisica Cosmica; Italia
Fil: Reynaldi, María Victoria. Instituto de Astrofísica de la Plata (conicet- Universidad Nacional de la Plata); Argentina
Fil: Vieyro, Florencia Laura. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Saponara, Juliana. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Andruchow, Ileana. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Lopez, I. E.. Istituto Di Astrofisica Spaziale E Fisica Cosmica; Italia
Fil: Benaglia, Paula. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Cellone, Sergio Aldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Masetti, Nicola. Istituto Di Astrofisica Spaziale E Fisica Cosmica; Italia
Fil: Massaro, F.. Universita Di Torino. Dipartimento Di Física Generale; Italia
Fil: Peña Herazo, H. A.. East Asian Observatory; Estados Unidos
Fil: Chavushyan, Vahram. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Combi, Jorge Ariel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Acosta Pulido, J. A.. Instituto de Astrofisica de Canarias; España
Fil: Agis Gonzalez, B.. Instituto de Astrofísica de Andalucía; España
Fil: Castro Segura, N.. University of Southampton; Reino Unido
Materia
GALAXIES: ACTIVE
GALAXIES: NUCLEI
GALAXIES:JETS
BL LACERTAE OBJECTS: GENERAL
X-RAYS: GALAXIES
GAMMA-RAYS: GALAXIES
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:11336/203811
Acceder
id CONICETDig_fefd10a8371346d7374d8cb95f2d2afb
oai_identifier_str oai:ri.conicet.gov.ar:11336/203811
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2Marchesini, Ezequiel JoaquínReynaldi, María VictoriaVieyro, Florencia LauraSaponara, JulianaAndruchow, IleanaLopez, I. E.Benaglia, PaulaCellone, Sergio AldoMasetti, NicolaMassaro, F.Peña Herazo, H. A.Chavushyan, VahramCombi, Jorge ArielAcosta Pulido, J. A.Agis Gonzalez, B.Castro Segura, N.GALAXIES: ACTIVEGALAXIES: NUCLEIGALAXIES:JETSBL LACERTAE OBJECTS: GENERALX-RAYS: GALAXIESGAMMA-RAYS: GALAXIEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. The gamma-ray emitting source WISE J141046.00+740511.2 has been associated with a Fermi-LAT detection by crossmatching with Swift/XRT data. It has shown all the canonical observational characteristics of a BL Lac source, including a power-law, featureless optical spectrum. However, it was only recently detected at radio frequencies and its radio flux is significantly low. Aims. Given that a radio detection is fundamental to associate lower-energy counterparts to Fermi-LAT sources, we aim to unambiguously classify this source by performing a multiwavelength analysis based on contemporaneous data. Methods. By using multifrequency observations at the Jansky Very Large Array, Giant Metrewave Radio Telescope, Gran Telescopio Canarias, Gemini, William Herschel Telescope and Liverpool observatories, together with Fermi-LAT and Swift data, we carried out two kinds of analyses. On one hand, we studied several known parameters that account for the radio loudness or weakness characterization and their application to blazars (in general) and to our source (in particular). And, on the other hand, we built and analyzed the observed spectral energy distribution (SED) of this source to try to explain its peculiar characteristics. Results. The multiwavelength analysis indicates that WISE J141046.00+740511.2 is a blazar of the high-frequency peaked (HBL) type that emits highly polarized light and that is likely located at a low redshift. In addition, the one-zone model parameters that best fit its SED are those of an extreme HBL (EHBL); this blazar type has been extensively predicted in theory to be lacking in the radio emission that is otherwise typical of canonical gamma-ray blazars. Conclusions. We confirm that WISE J141046.00+740511.2 is indeed a highly polarized BL Lac of the HBL type. Further studies will be conducted to explain the atypical low radio flux detected for this source.Fil: Marchesini, Ezequiel Joaquín. Istituto Di Astrofisica Spaziale E Fisica Cosmica; ItaliaFil: Reynaldi, María Victoria. Instituto de Astrofísica de la Plata (conicet- Universidad Nacional de la Plata); ArgentinaFil: Vieyro, Florencia Laura. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Saponara, Juliana. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Andruchow, Ileana. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Lopez, I. E.. Istituto Di Astrofisica Spaziale E Fisica Cosmica; ItaliaFil: Benaglia, Paula. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Cellone, Sergio Aldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaFil: Masetti, Nicola. Istituto Di Astrofisica Spaziale E Fisica Cosmica; ItaliaFil: Massaro, F.. Universita Di Torino. Dipartimento Di Física Generale; ItaliaFil: Peña Herazo, H. A.. East Asian Observatory; Estados UnidosFil: Chavushyan, Vahram. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Combi, Jorge Ariel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Acosta Pulido, J. A.. Instituto de Astrofisica de Canarias; EspañaFil: Agis Gonzalez, B.. Instituto de Astrofísica de Andalucía; EspañaFil: Castro Segura, N.. University of Southampton; Reino UnidoEDP Sciences2022-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/203811Marchesini, Ezequiel Joaquín; Reynaldi, María Victoria; Vieyro, Florencia Laura; Saponara, Juliana; Andruchow, Ileana; et al.; Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2; EDP Sciences; Astronomy and Astrophysics; 670; a91; 11-2022; 1-130004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/10.1051/0004-6361/202244899info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202244899info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:54:42Zoai:ri.conicet.gov.ar:11336/203811instacron: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:34982025-09-03 09:54:43.109CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2
title Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2
spellingShingle Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2
Marchesini, Ezequiel Joaquín
GALAXIES: ACTIVE
GALAXIES: NUCLEI
GALAXIES:JETS
BL LACERTAE OBJECTS: GENERAL
X-RAYS: GALAXIES
GAMMA-RAYS: GALAXIES
title_short Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2
title_full Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2
title_fullStr Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2
title_full_unstemmed Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2
title_sort Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2
dc.creator.none.fl_str_mv Marchesini, Ezequiel Joaquín
Reynaldi, María Victoria
Vieyro, Florencia Laura
Saponara, Juliana
Andruchow, Ileana
Lopez, I. E.
Benaglia, Paula
Cellone, Sergio Aldo
Masetti, Nicola
Massaro, F.
Peña Herazo, H. A.
Chavushyan, Vahram
Combi, Jorge Ariel
Acosta Pulido, J. A.
Agis Gonzalez, B.
Castro Segura, N.
author Marchesini, Ezequiel Joaquín
author_facet Marchesini, Ezequiel Joaquín
Reynaldi, María Victoria
Vieyro, Florencia Laura
Saponara, Juliana
Andruchow, Ileana
Lopez, I. E.
Benaglia, Paula
Cellone, Sergio Aldo
Masetti, Nicola
Massaro, F.
Peña Herazo, H. A.
Chavushyan, Vahram
Combi, Jorge Ariel
Acosta Pulido, J. A.
Agis Gonzalez, B.
Castro Segura, N.
author_role author
author2 Reynaldi, María Victoria
Vieyro, Florencia Laura
Saponara, Juliana
Andruchow, Ileana
Lopez, I. E.
Benaglia, Paula
Cellone, Sergio Aldo
Masetti, Nicola
Massaro, F.
Peña Herazo, H. A.
Chavushyan, Vahram
Combi, Jorge Ariel
Acosta Pulido, J. A.
Agis Gonzalez, B.
Castro Segura, N.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv GALAXIES: ACTIVE
GALAXIES: NUCLEI
GALAXIES:JETS
BL LACERTAE OBJECTS: GENERAL
X-RAYS: GALAXIES
GAMMA-RAYS: GALAXIES
topic GALAXIES: ACTIVE
GALAXIES: NUCLEI
GALAXIES:JETS
BL LACERTAE OBJECTS: GENERAL
X-RAYS: GALAXIES
GAMMA-RAYS: GALAXIES
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. The gamma-ray emitting source WISE J141046.00+740511.2 has been associated with a Fermi-LAT detection by crossmatching with Swift/XRT data. It has shown all the canonical observational characteristics of a BL Lac source, including a power-law, featureless optical spectrum. However, it was only recently detected at radio frequencies and its radio flux is significantly low. Aims. Given that a radio detection is fundamental to associate lower-energy counterparts to Fermi-LAT sources, we aim to unambiguously classify this source by performing a multiwavelength analysis based on contemporaneous data. Methods. By using multifrequency observations at the Jansky Very Large Array, Giant Metrewave Radio Telescope, Gran Telescopio Canarias, Gemini, William Herschel Telescope and Liverpool observatories, together with Fermi-LAT and Swift data, we carried out two kinds of analyses. On one hand, we studied several known parameters that account for the radio loudness or weakness characterization and their application to blazars (in general) and to our source (in particular). And, on the other hand, we built and analyzed the observed spectral energy distribution (SED) of this source to try to explain its peculiar characteristics. Results. The multiwavelength analysis indicates that WISE J141046.00+740511.2 is a blazar of the high-frequency peaked (HBL) type that emits highly polarized light and that is likely located at a low redshift. In addition, the one-zone model parameters that best fit its SED are those of an extreme HBL (EHBL); this blazar type has been extensively predicted in theory to be lacking in the radio emission that is otherwise typical of canonical gamma-ray blazars. Conclusions. We confirm that WISE J141046.00+740511.2 is indeed a highly polarized BL Lac of the HBL type. Further studies will be conducted to explain the atypical low radio flux detected for this source.
Fil: Marchesini, Ezequiel Joaquín. Istituto Di Astrofisica Spaziale E Fisica Cosmica; Italia
Fil: Reynaldi, María Victoria. Instituto de Astrofísica de la Plata (conicet- Universidad Nacional de la Plata); Argentina
Fil: Vieyro, Florencia Laura. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Saponara, Juliana. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Andruchow, Ileana. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Lopez, I. E.. Istituto Di Astrofisica Spaziale E Fisica Cosmica; Italia
Fil: Benaglia, Paula. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Cellone, Sergio Aldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Masetti, Nicola. Istituto Di Astrofisica Spaziale E Fisica Cosmica; Italia
Fil: Massaro, F.. Universita Di Torino. Dipartimento Di Física Generale; Italia
Fil: Peña Herazo, H. A.. East Asian Observatory; Estados Unidos
Fil: Chavushyan, Vahram. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Combi, Jorge Ariel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Acosta Pulido, J. A.. Instituto de Astrofisica de Canarias; España
Fil: Agis Gonzalez, B.. Instituto de Astrofísica de Andalucía; España
Fil: Castro Segura, N.. University of Southampton; Reino Unido
description Context. The gamma-ray emitting source WISE J141046.00+740511.2 has been associated with a Fermi-LAT detection by crossmatching with Swift/XRT data. It has shown all the canonical observational characteristics of a BL Lac source, including a power-law, featureless optical spectrum. However, it was only recently detected at radio frequencies and its radio flux is significantly low. Aims. Given that a radio detection is fundamental to associate lower-energy counterparts to Fermi-LAT sources, we aim to unambiguously classify this source by performing a multiwavelength analysis based on contemporaneous data. Methods. By using multifrequency observations at the Jansky Very Large Array, Giant Metrewave Radio Telescope, Gran Telescopio Canarias, Gemini, William Herschel Telescope and Liverpool observatories, together with Fermi-LAT and Swift data, we carried out two kinds of analyses. On one hand, we studied several known parameters that account for the radio loudness or weakness characterization and their application to blazars (in general) and to our source (in particular). And, on the other hand, we built and analyzed the observed spectral energy distribution (SED) of this source to try to explain its peculiar characteristics. Results. The multiwavelength analysis indicates that WISE J141046.00+740511.2 is a blazar of the high-frequency peaked (HBL) type that emits highly polarized light and that is likely located at a low redshift. In addition, the one-zone model parameters that best fit its SED are those of an extreme HBL (EHBL); this blazar type has been extensively predicted in theory to be lacking in the radio emission that is otherwise typical of canonical gamma-ray blazars. Conclusions. We confirm that WISE J141046.00+740511.2 is indeed a highly polarized BL Lac of the HBL type. Further studies will be conducted to explain the atypical low radio flux detected for this source.
publishDate 2022
dc.date.none.fl_str_mv 2022-11
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/11336/203811
Marchesini, Ezequiel Joaquín; Reynaldi, María Victoria; Vieyro, Florencia Laura; Saponara, Juliana; Andruchow, Ileana; et al.; Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2; EDP Sciences; Astronomy and Astrophysics; 670; a91; 11-2022; 1-13
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/203811
identifier_str_mv Marchesini, Ezequiel Joaquín; Reynaldi, María Victoria; Vieyro, Florencia Laura; Saponara, Juliana; Andruchow, Ileana; et al.; Disentangling the nature of the first radio weak BL Lac: Contemporaneous multifrequency observations of WISE J141046.00+740511.2; EDP Sciences; Astronomy and Astrophysics; 670; a91; 11-2022; 1-13
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/10.1051/0004-6361/202244899
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202244899
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
application/pdf
application/pdf
application/pdf
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_ 1842269302337568768
score 13.13397

Publicaciones similares