The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release
- Autores
- Kitaura, Francisco-Shu; Rodriguez Torres, Sergio A.; Chuang, Chia Hsun; Zhao, Cheng; Prada, Francisco; Gil Marín, Héctor; Guo, Hong; Yepes, Gustavo; Klypin, Anatoly; Scoccola, Claudia Graciela; Tinker, Jeremy; McBride, Cameron; Reid, Beth; Sánchez, Ariel G.; Salazar Albornoz, Salvador; Grieb, Jan Niklas; Vargas Magana, Mariana; Cuesta, Antonio J.; Neyrinck, Mark; Beutler, Florian; Comparat, Johan; Percival, Will J.; Ross, Ashley
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation Spectroscopic Survey Final Data Release (BOSS DR11 and DR12) with high fidelity on all relevant scales in order to allow a robust analysis of baryon acoustic oscillations and redshift space distortions. We have generated (6000) 12 288 MultiDark PATCHY BOSS (DR11) DR12 light cones corresponding to an effective volume of ~ 192 000 [h-1 Gpc]3 (the largest ever simulated volume), including cosmic evolution in the redshift range from 0.15 to 0.75. The mocks have been calibrated using a reference galaxy catalogue based on the halo abundance matching modelling of the BOSS DR11 and DR12 galaxy clustering data and on the data themselves. The production follows three steps. First, we apply the PATCHY code to generate a dark matter field and an object distribution including non-linear stochastic galaxy bias. Secondly, we run the halo/stellar distribution reconstruction HADRON code to assign masses to the various objects. This step uses the mass distribution as a function of local density and non-local indicators (i.e. tidal field tensor eigenvalues and relative halo exclusion separation for massive objects) from the reference simulation applied to the corresponding patchy dark matter and galaxy distribution. Finally, we apply the SUGAR code to build the light cones. The resulting MultiDarkPATCHY mock light cones reproduce the number density, selection function, survey geometry, and in general within 1s, for arbitrary stellar mass bins, the power spectrum up to k = 0.3 h Mpc-1, the two-point correlation functions down to a few Mpc scales, and the three-point statistics of the BOSS DR11 and DR12 galaxy samples.
Fil: Kitaura, Francisco-Shu. Leibniz-Institut für Astrophysik Potsdam; Alemania
Fil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; España
Fil: Chuang, Chia Hsun. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; España
Fil: Zhao, Cheng. Tsinghua University; China
Fil: Prada, Francisco. Consejo Superior de Investigaciones Científicas; España. Universidad Autónoma de Madrid; España
Fil: Gil Marín, Héctor. University of Portsmouth; Reino Unido
Fil: Guo, Hong. State University of Utah; Estados Unidos. Shanghai Astronomical Observatory; China
Fil: Yepes, Gustavo. Universidad Autónoma de Madrid. Facultad de Ciencias; España
Fil: Klypin, Anatoly. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; España. New Mexico State University; Estados Unidos
Fil: Scoccola, Claudia Graciela. Universidad Autónoma de Madrid; España. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina. Instituto de Astrof{isica de Canarias; España. Universidad de La Laguna; España
Fil: Tinker, Jeremy. University of New York; Estados Unidos
Fil: McBride, Cameron. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Reid, Beth. Lawrence Berkeley National Laboratory; Estados Unidos. University of California at Berkeley; Estados Unidos
Fil: Sánchez, Ariel G.. Max Planck Institut für Extraterrestrische Physik; Alemania
Fil: Salazar Albornoz, Salvador. Max Planck Institut für Extraterrestrische Physik; Alemania. Ludwig Maximilians Universitat; Alemania
Fil: Grieb, Jan Niklas. Max Planck Institut für Extraterrestrische Physik; Alemania. Ludwig Maximilians Universitat; Alemania
Fil: Vargas Magana, Mariana. Universidad Nacional Autónoma de México; México
Fil: Cuesta, Antonio J.. Universidad de Barcelona; España
Fil: Neyrinck, Mark. University Johns Hopkins; Estados Unidos
Fil: Beutler, Florian. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Comparat, Johan. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; España
Fil: Percival, Will J.. University of Portsmouth; Reino Unido
Fil: Ross, Ashley. Ohio State University; Estados Unidos. University of Portsmouth; Reino Unido - Materia
-
GALAXIES: HALOES
GALAXIES: STATISTICS
LARGE-SCALE STRUCTURE OF UNIVERSE
METHODS: NUMERICAL - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/79187
Ver los metadatos del registro completo
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data ReleaseKitaura, Francisco-ShuRodriguez Torres, Sergio A.Chuang, Chia HsunZhao, ChengPrada, FranciscoGil Marín, HéctorGuo, HongYepes, GustavoKlypin, AnatolyScoccola, Claudia GracielaTinker, JeremyMcBride, CameronReid, BethSánchez, Ariel G.Salazar Albornoz, SalvadorGrieb, Jan NiklasVargas Magana, MarianaCuesta, Antonio J.Neyrinck, MarkBeutler, FlorianComparat, JohanPercival, Will J.Ross, AshleyGALAXIES: HALOESGALAXIES: STATISTICSLARGE-SCALE STRUCTURE OF UNIVERSEMETHODS: NUMERICALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation Spectroscopic Survey Final Data Release (BOSS DR11 and DR12) with high fidelity on all relevant scales in order to allow a robust analysis of baryon acoustic oscillations and redshift space distortions. We have generated (6000) 12 288 MultiDark PATCHY BOSS (DR11) DR12 light cones corresponding to an effective volume of ~ 192 000 [h-1 Gpc]3 (the largest ever simulated volume), including cosmic evolution in the redshift range from 0.15 to 0.75. The mocks have been calibrated using a reference galaxy catalogue based on the halo abundance matching modelling of the BOSS DR11 and DR12 galaxy clustering data and on the data themselves. The production follows three steps. First, we apply the PATCHY code to generate a dark matter field and an object distribution including non-linear stochastic galaxy bias. Secondly, we run the halo/stellar distribution reconstruction HADRON code to assign masses to the various objects. This step uses the mass distribution as a function of local density and non-local indicators (i.e. tidal field tensor eigenvalues and relative halo exclusion separation for massive objects) from the reference simulation applied to the corresponding patchy dark matter and galaxy distribution. Finally, we apply the SUGAR code to build the light cones. The resulting MultiDarkPATCHY mock light cones reproduce the number density, selection function, survey geometry, and in general within 1s, for arbitrary stellar mass bins, the power spectrum up to k = 0.3 h Mpc-1, the two-point correlation functions down to a few Mpc scales, and the three-point statistics of the BOSS DR11 and DR12 galaxy samples.Fil: Kitaura, Francisco-Shu. Leibniz-Institut für Astrophysik Potsdam; AlemaniaFil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; EspañaFil: Chuang, Chia Hsun. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; EspañaFil: Zhao, Cheng. Tsinghua University; ChinaFil: Prada, Francisco. Consejo Superior de Investigaciones Científicas; España. Universidad Autónoma de Madrid; EspañaFil: Gil Marín, Héctor. University of Portsmouth; Reino UnidoFil: Guo, Hong. State University of Utah; Estados Unidos. Shanghai Astronomical Observatory; ChinaFil: Yepes, Gustavo. Universidad Autónoma de Madrid. Facultad de Ciencias; EspañaFil: Klypin, Anatoly. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; España. New Mexico State University; Estados UnidosFil: Scoccola, Claudia Graciela. Universidad Autónoma de Madrid; España. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina. Instituto de Astrof{isica de Canarias; España. Universidad de La Laguna; EspañaFil: Tinker, Jeremy. University of New York; Estados UnidosFil: McBride, Cameron. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Reid, Beth. Lawrence Berkeley National Laboratory; Estados Unidos. University of California at Berkeley; Estados UnidosFil: Sánchez, Ariel G.. Max Planck Institut für Extraterrestrische Physik; AlemaniaFil: Salazar Albornoz, Salvador. Max Planck Institut für Extraterrestrische Physik; Alemania. Ludwig Maximilians Universitat; AlemaniaFil: Grieb, Jan Niklas. Max Planck Institut für Extraterrestrische Physik; Alemania. Ludwig Maximilians Universitat; AlemaniaFil: Vargas Magana, Mariana. Universidad Nacional Autónoma de México; MéxicoFil: Cuesta, Antonio J.. Universidad de Barcelona; EspañaFil: Neyrinck, Mark. University Johns Hopkins; Estados UnidosFil: Beutler, Florian. Lawrence Berkeley National Laboratory; Estados UnidosFil: Comparat, Johan. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; EspañaFil: Percival, Will J.. University of Portsmouth; Reino UnidoFil: Ross, Ashley. Ohio State University; Estados Unidos. University of Portsmouth; Reino UnidoWiley Blackwell Publishing, Inc2016-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/79187Kitaura, Francisco-Shu; Rodriguez Torres, Sergio A.; Chuang, Chia Hsun; Zhao, Cheng; Prada, Francisco; et al.; The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 456; 4; 3-2016; 4156-41730035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stv2826info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/456/4/4156/2892161info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1509.06400info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T12:14:19Zoai:ri.conicet.gov.ar:11336/79187instacron: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 12:14:20.096CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| title |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| spellingShingle |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release Kitaura, Francisco-Shu GALAXIES: HALOES GALAXIES: STATISTICS LARGE-SCALE STRUCTURE OF UNIVERSE METHODS: NUMERICAL |
| title_short |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| title_full |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| title_fullStr |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| title_full_unstemmed |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| title_sort |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release |
| dc.creator.none.fl_str_mv |
Kitaura, Francisco-Shu Rodriguez Torres, Sergio A. Chuang, Chia Hsun Zhao, Cheng Prada, Francisco Gil Marín, Héctor Guo, Hong Yepes, Gustavo Klypin, Anatoly Scoccola, Claudia Graciela Tinker, Jeremy McBride, Cameron Reid, Beth Sánchez, Ariel G. Salazar Albornoz, Salvador Grieb, Jan Niklas Vargas Magana, Mariana Cuesta, Antonio J. Neyrinck, Mark Beutler, Florian Comparat, Johan Percival, Will J. Ross, Ashley |
| author |
Kitaura, Francisco-Shu |
| author_facet |
Kitaura, Francisco-Shu Rodriguez Torres, Sergio A. Chuang, Chia Hsun Zhao, Cheng Prada, Francisco Gil Marín, Héctor Guo, Hong Yepes, Gustavo Klypin, Anatoly Scoccola, Claudia Graciela Tinker, Jeremy McBride, Cameron Reid, Beth Sánchez, Ariel G. Salazar Albornoz, Salvador Grieb, Jan Niklas Vargas Magana, Mariana Cuesta, Antonio J. Neyrinck, Mark Beutler, Florian Comparat, Johan Percival, Will J. Ross, Ashley |
| author_role |
author |
| author2 |
Rodriguez Torres, Sergio A. Chuang, Chia Hsun Zhao, Cheng Prada, Francisco Gil Marín, Héctor Guo, Hong Yepes, Gustavo Klypin, Anatoly Scoccola, Claudia Graciela Tinker, Jeremy McBride, Cameron Reid, Beth Sánchez, Ariel G. Salazar Albornoz, Salvador Grieb, Jan Niklas Vargas Magana, Mariana Cuesta, Antonio J. Neyrinck, Mark Beutler, Florian Comparat, Johan Percival, Will J. Ross, Ashley |
| author2_role |
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 |
GALAXIES: HALOES GALAXIES: STATISTICS LARGE-SCALE STRUCTURE OF UNIVERSE METHODS: NUMERICAL |
| topic |
GALAXIES: HALOES GALAXIES: STATISTICS LARGE-SCALE STRUCTURE OF UNIVERSE METHODS: NUMERICAL |
| 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 reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation Spectroscopic Survey Final Data Release (BOSS DR11 and DR12) with high fidelity on all relevant scales in order to allow a robust analysis of baryon acoustic oscillations and redshift space distortions. We have generated (6000) 12 288 MultiDark PATCHY BOSS (DR11) DR12 light cones corresponding to an effective volume of ~ 192 000 [h-1 Gpc]3 (the largest ever simulated volume), including cosmic evolution in the redshift range from 0.15 to 0.75. The mocks have been calibrated using a reference galaxy catalogue based on the halo abundance matching modelling of the BOSS DR11 and DR12 galaxy clustering data and on the data themselves. The production follows three steps. First, we apply the PATCHY code to generate a dark matter field and an object distribution including non-linear stochastic galaxy bias. Secondly, we run the halo/stellar distribution reconstruction HADRON code to assign masses to the various objects. This step uses the mass distribution as a function of local density and non-local indicators (i.e. tidal field tensor eigenvalues and relative halo exclusion separation for massive objects) from the reference simulation applied to the corresponding patchy dark matter and galaxy distribution. Finally, we apply the SUGAR code to build the light cones. The resulting MultiDarkPATCHY mock light cones reproduce the number density, selection function, survey geometry, and in general within 1s, for arbitrary stellar mass bins, the power spectrum up to k = 0.3 h Mpc-1, the two-point correlation functions down to a few Mpc scales, and the three-point statistics of the BOSS DR11 and DR12 galaxy samples. Fil: Kitaura, Francisco-Shu. Leibniz-Institut für Astrophysik Potsdam; Alemania Fil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; España Fil: Chuang, Chia Hsun. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; España Fil: Zhao, Cheng. Tsinghua University; China Fil: Prada, Francisco. Consejo Superior de Investigaciones Científicas; España. Universidad Autónoma de Madrid; España Fil: Gil Marín, Héctor. University of Portsmouth; Reino Unido Fil: Guo, Hong. State University of Utah; Estados Unidos. Shanghai Astronomical Observatory; China Fil: Yepes, Gustavo. Universidad Autónoma de Madrid. Facultad de Ciencias; España Fil: Klypin, Anatoly. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; España. New Mexico State University; Estados Unidos Fil: Scoccola, Claudia Graciela. Universidad Autónoma de Madrid; España. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina. Instituto de Astrof{isica de Canarias; España. Universidad de La Laguna; España Fil: Tinker, Jeremy. University of New York; Estados Unidos Fil: McBride, Cameron. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Reid, Beth. Lawrence Berkeley National Laboratory; Estados Unidos. University of California at Berkeley; Estados Unidos Fil: Sánchez, Ariel G.. Max Planck Institut für Extraterrestrische Physik; Alemania Fil: Salazar Albornoz, Salvador. Max Planck Institut für Extraterrestrische Physik; Alemania. Ludwig Maximilians Universitat; Alemania Fil: Grieb, Jan Niklas. Max Planck Institut für Extraterrestrische Physik; Alemania. Ludwig Maximilians Universitat; Alemania Fil: Vargas Magana, Mariana. Universidad Nacional Autónoma de México; México Fil: Cuesta, Antonio J.. Universidad de Barcelona; España Fil: Neyrinck, Mark. University Johns Hopkins; Estados Unidos Fil: Beutler, Florian. Lawrence Berkeley National Laboratory; Estados Unidos Fil: Comparat, Johan. Universidad Autónoma de Madrid; España. Consejo Superior de Investigaciones Científicas; España Fil: Percival, Will J.. University of Portsmouth; Reino Unido Fil: Ross, Ashley. Ohio State University; Estados Unidos. University of Portsmouth; Reino Unido |
| description |
We reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation Spectroscopic Survey Final Data Release (BOSS DR11 and DR12) with high fidelity on all relevant scales in order to allow a robust analysis of baryon acoustic oscillations and redshift space distortions. We have generated (6000) 12 288 MultiDark PATCHY BOSS (DR11) DR12 light cones corresponding to an effective volume of ~ 192 000 [h-1 Gpc]3 (the largest ever simulated volume), including cosmic evolution in the redshift range from 0.15 to 0.75. The mocks have been calibrated using a reference galaxy catalogue based on the halo abundance matching modelling of the BOSS DR11 and DR12 galaxy clustering data and on the data themselves. The production follows three steps. First, we apply the PATCHY code to generate a dark matter field and an object distribution including non-linear stochastic galaxy bias. Secondly, we run the halo/stellar distribution reconstruction HADRON code to assign masses to the various objects. This step uses the mass distribution as a function of local density and non-local indicators (i.e. tidal field tensor eigenvalues and relative halo exclusion separation for massive objects) from the reference simulation applied to the corresponding patchy dark matter and galaxy distribution. Finally, we apply the SUGAR code to build the light cones. The resulting MultiDarkPATCHY mock light cones reproduce the number density, selection function, survey geometry, and in general within 1s, for arbitrary stellar mass bins, the power spectrum up to k = 0.3 h Mpc-1, the two-point correlation functions down to a few Mpc scales, and the three-point statistics of the BOSS DR11 and DR12 galaxy samples. |
| publishDate |
2016 |
| dc.date.none.fl_str_mv |
2016-03 |
| 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/11336/79187 Kitaura, Francisco-Shu; Rodriguez Torres, Sergio A.; Chuang, Chia Hsun; Zhao, Cheng; Prada, Francisco; et al.; The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 456; 4; 3-2016; 4156-4173 0035-8711 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/79187 |
| identifier_str_mv |
Kitaura, Francisco-Shu; Rodriguez Torres, Sergio A.; Chuang, Chia Hsun; Zhao, Cheng; Prada, Francisco; et al.; The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Mock galaxy catalogues for the BOSS Final Data Release; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 456; 4; 3-2016; 4156-4173 0035-8711 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
| dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stv2826 info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/456/4/4156/2892161 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1509.06400 |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/ |
| eu_rights_str_mv |
openAccess |
| rights_invalid_str_mv |
https://creativecommons.org/licenses/by/2.5/ar/ |
| dc.format.none.fl_str_mv |
application/pdf application/pdf application/pdf |
| dc.publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
| publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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