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
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/79187

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network_name_str CONICET Digital (CONICET)
spelling 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 Técnicas2025-09-29T10:41:43Zoai: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:34982025-09-29 10:41:43.781CONICET 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
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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