European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters

Autores
Vázquez Ramió, Héctor; Vernin, Jean; Muñoz Tuñon, Casiana; Sarazin, Marc; Varela, Antonia M.; Trinquet, Hervé; Delgado, José Miguel; Fuensalida, Jesús J.; Reyes, Marcos; Benhida, Abdelmajid; Benkhaldoun, Zouhair; Garcia Lambas, Diego Rodolfo; Hach, Youssef; Lazrek, M.; Lombardi, Gianluca; Navarrete, Julio; Recabarren, Pablo Genaro Antonio; Renzi, Victor Alberto; Sabil, Mohammed; Vrech, Ruben Hector
Año de publicación
2012
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
This is the second article of a series devoted to European Extremely Large Telescope (E-ELT) site characterization. In this article we present the main properties of the parameters involved in high angular resolution observations from the data collected in the site testing campaign of the E-ELT during the design study (DS) phase. Observations were made in 2008 and 2009, in the four sites selected to shelter the future E-ELT (characterized under the ELT-DS contract): Aklim mountain in Morocco, Observatorio del Roque de los Muchachos (ORM) in Spain, Macón range in Argentina, and Cerro Ventarrones in Chile. The same techniques, instruments, and acquisition procedures were taken on each site. A multiple aperture scintillation sensor (MASS) and a differential image motion monitor (DIMM) were installed at each site. Global statistics of the integrated seeing, the free atmosphere seeing, the boundary layer seeing, and the isoplanatic angle were studied for each site, and the results are presented here. In order to estimate other important parameters, such as the coherence time of the wavefront and the overall parameter “coherence étendue,” additional information of vertical profiles of the wind speed was needed. Data were retrieved from the National Oceanic and Atmospheric Administration (NOAA) archive. Ground wind speed was measured by automatic weather stations (AWS). More aspects of the turbulence parameters, such as their seasonal trend, their nightly evolution, and their temporal stability, were also obtained and analyzed.
Fil: Vázquez Ramió, Héctor. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; España
Fil: Vernin, Jean. Université de Nice-Sophia Antipolis; Francia
Fil: Muñoz Tuñon, Casiana. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; España
Fil: Sarazin, Marc. European Southern Observatory; Alemania
Fil: Varela, Antonia M.. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; España
Fil: Trinquet, Hervé. No especifíca;
Fil: Delgado, José Miguel. Instituto de Astrofísica de Canarias; España
Fil: Fuensalida, Jesús J.. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; España
Fil: Reyes, Marcos. Instituto de Astrofísica de Canarias; España
Fil: Benhida, Abdelmajid. Université Cadi Ayyad; Marruecos
Fil: Benkhaldoun, Zouhair. Université Cadi Ayyad; Marruecos
Fil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Hach, Youssef. Université Cadi Ayyad; Marruecos
Fil: Lazrek, M.. Université Cadi Ayyad; Marruecos
Fil: Lombardi, Gianluca. European Southern Observatory; Alemania
Fil: Navarrete, Julio. European Southern Observatory; Alemania
Fil: Recabarren, Pablo Genaro Antonio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Renzi, Victor Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Sabil, Mohammed. Université Cadi Ayyad; Marruecos
Fil: Vrech, Ruben Hector. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Materia
TELESCOPE
CHARACTERIZATION
OBSERVATIONS
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:11336/272710

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network_name_str CONICET Digital (CONICET)
spelling European Extremely Large Telescope Site Characterization. II. High Angular Resolution ParametersVázquez Ramió, HéctorVernin, JeanMuñoz Tuñon, CasianaSarazin, MarcVarela, Antonia M.Trinquet, HervéDelgado, José MiguelFuensalida, Jesús J.Reyes, MarcosBenhida, AbdelmajidBenkhaldoun, ZouhairGarcia Lambas, Diego RodolfoHach, YoussefLazrek, M.Lombardi, GianlucaNavarrete, JulioRecabarren, Pablo Genaro AntonioRenzi, Victor AlbertoSabil, MohammedVrech, Ruben HectorTELESCOPECHARACTERIZATIONOBSERVATIONShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1This is the second article of a series devoted to European Extremely Large Telescope (E-ELT) site characterization. In this article we present the main properties of the parameters involved in high angular resolution observations from the data collected in the site testing campaign of the E-ELT during the design study (DS) phase. Observations were made in 2008 and 2009, in the four sites selected to shelter the future E-ELT (characterized under the ELT-DS contract): Aklim mountain in Morocco, Observatorio del Roque de los Muchachos (ORM) in Spain, Macón range in Argentina, and Cerro Ventarrones in Chile. The same techniques, instruments, and acquisition procedures were taken on each site. A multiple aperture scintillation sensor (MASS) and a differential image motion monitor (DIMM) were installed at each site. Global statistics of the integrated seeing, the free atmosphere seeing, the boundary layer seeing, and the isoplanatic angle were studied for each site, and the results are presented here. In order to estimate other important parameters, such as the coherence time of the wavefront and the overall parameter “coherence étendue,” additional information of vertical profiles of the wind speed was needed. Data were retrieved from the National Oceanic and Atmospheric Administration (NOAA) archive. Ground wind speed was measured by automatic weather stations (AWS). More aspects of the turbulence parameters, such as their seasonal trend, their nightly evolution, and their temporal stability, were also obtained and analyzed.Fil: Vázquez Ramió, Héctor. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; EspañaFil: Vernin, Jean. Université de Nice-Sophia Antipolis; FranciaFil: Muñoz Tuñon, Casiana. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; EspañaFil: Sarazin, Marc. European Southern Observatory; AlemaniaFil: Varela, Antonia M.. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; EspañaFil: Trinquet, Hervé. No especifíca;Fil: Delgado, José Miguel. Instituto de Astrofísica de Canarias; EspañaFil: Fuensalida, Jesús J.. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; EspañaFil: Reyes, Marcos. Instituto de Astrofísica de Canarias; EspañaFil: Benhida, Abdelmajid. Université Cadi Ayyad; MarruecosFil: Benkhaldoun, Zouhair. Université Cadi Ayyad; MarruecosFil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Hach, Youssef. Université Cadi Ayyad; MarruecosFil: Lazrek, M.. Université Cadi Ayyad; MarruecosFil: Lombardi, Gianluca. European Southern Observatory; AlemaniaFil: Navarrete, Julio. European Southern Observatory; AlemaniaFil: Recabarren, Pablo Genaro Antonio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Renzi, Victor Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Sabil, Mohammed. Université Cadi Ayyad; MarruecosFil: Vrech, Ruben Hector. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaUniversity of Chicago Press2012-08info: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/11336/272710Vázquez Ramió, Héctor; Vernin, Jean; Muñoz Tuñon, Casiana; Sarazin, Marc; Varela, Antonia M.; et al.; European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters; University of Chicago Press; Publications of the Astronomical Society of the Pacific; 124; 918; 8-2012; 868-8840004-6280CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/667599info:eu-repo/semantics/altIdentifier/doi/10.1086/667599info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-11-05T10:40:23Zoai:ri.conicet.gov.ar:11336/272710instacron: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:34982025-11-05 10:40:23.681CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters
title European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters
spellingShingle European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters
Vázquez Ramió, Héctor
TELESCOPE
CHARACTERIZATION
OBSERVATIONS
title_short European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters
title_full European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters
title_fullStr European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters
title_full_unstemmed European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters
title_sort European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters
dc.creator.none.fl_str_mv Vázquez Ramió, Héctor
Vernin, Jean
Muñoz Tuñon, Casiana
Sarazin, Marc
Varela, Antonia M.
Trinquet, Hervé
Delgado, José Miguel
Fuensalida, Jesús J.
Reyes, Marcos
Benhida, Abdelmajid
Benkhaldoun, Zouhair
Garcia Lambas, Diego Rodolfo
Hach, Youssef
Lazrek, M.
Lombardi, Gianluca
Navarrete, Julio
Recabarren, Pablo Genaro Antonio
Renzi, Victor Alberto
Sabil, Mohammed
Vrech, Ruben Hector
author Vázquez Ramió, Héctor
author_facet Vázquez Ramió, Héctor
Vernin, Jean
Muñoz Tuñon, Casiana
Sarazin, Marc
Varela, Antonia M.
Trinquet, Hervé
Delgado, José Miguel
Fuensalida, Jesús J.
Reyes, Marcos
Benhida, Abdelmajid
Benkhaldoun, Zouhair
Garcia Lambas, Diego Rodolfo
Hach, Youssef
Lazrek, M.
Lombardi, Gianluca
Navarrete, Julio
Recabarren, Pablo Genaro Antonio
Renzi, Victor Alberto
Sabil, Mohammed
Vrech, Ruben Hector
author_role author
author2 Vernin, Jean
Muñoz Tuñon, Casiana
Sarazin, Marc
Varela, Antonia M.
Trinquet, Hervé
Delgado, José Miguel
Fuensalida, Jesús J.
Reyes, Marcos
Benhida, Abdelmajid
Benkhaldoun, Zouhair
Garcia Lambas, Diego Rodolfo
Hach, Youssef
Lazrek, M.
Lombardi, Gianluca
Navarrete, Julio
Recabarren, Pablo Genaro Antonio
Renzi, Victor Alberto
Sabil, Mohammed
Vrech, Ruben Hector
author2_role 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 TELESCOPE
CHARACTERIZATION
OBSERVATIONS
topic TELESCOPE
CHARACTERIZATION
OBSERVATIONS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv This is the second article of a series devoted to European Extremely Large Telescope (E-ELT) site characterization. In this article we present the main properties of the parameters involved in high angular resolution observations from the data collected in the site testing campaign of the E-ELT during the design study (DS) phase. Observations were made in 2008 and 2009, in the four sites selected to shelter the future E-ELT (characterized under the ELT-DS contract): Aklim mountain in Morocco, Observatorio del Roque de los Muchachos (ORM) in Spain, Macón range in Argentina, and Cerro Ventarrones in Chile. The same techniques, instruments, and acquisition procedures were taken on each site. A multiple aperture scintillation sensor (MASS) and a differential image motion monitor (DIMM) were installed at each site. Global statistics of the integrated seeing, the free atmosphere seeing, the boundary layer seeing, and the isoplanatic angle were studied for each site, and the results are presented here. In order to estimate other important parameters, such as the coherence time of the wavefront and the overall parameter “coherence étendue,” additional information of vertical profiles of the wind speed was needed. Data were retrieved from the National Oceanic and Atmospheric Administration (NOAA) archive. Ground wind speed was measured by automatic weather stations (AWS). More aspects of the turbulence parameters, such as their seasonal trend, their nightly evolution, and their temporal stability, were also obtained and analyzed.
Fil: Vázquez Ramió, Héctor. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; España
Fil: Vernin, Jean. Université de Nice-Sophia Antipolis; Francia
Fil: Muñoz Tuñon, Casiana. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; España
Fil: Sarazin, Marc. European Southern Observatory; Alemania
Fil: Varela, Antonia M.. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; España
Fil: Trinquet, Hervé. No especifíca;
Fil: Delgado, José Miguel. Instituto de Astrofísica de Canarias; España
Fil: Fuensalida, Jesús J.. Universidad de La Laguna; España. Instituto de Astrofísica de Canarias; España
Fil: Reyes, Marcos. Instituto de Astrofísica de Canarias; España
Fil: Benhida, Abdelmajid. Université Cadi Ayyad; Marruecos
Fil: Benkhaldoun, Zouhair. Université Cadi Ayyad; Marruecos
Fil: Garcia Lambas, Diego Rodolfo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Hach, Youssef. Université Cadi Ayyad; Marruecos
Fil: Lazrek, M.. Université Cadi Ayyad; Marruecos
Fil: Lombardi, Gianluca. European Southern Observatory; Alemania
Fil: Navarrete, Julio. European Southern Observatory; Alemania
Fil: Recabarren, Pablo Genaro Antonio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Renzi, Victor Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Sabil, Mohammed. Université Cadi Ayyad; Marruecos
Fil: Vrech, Ruben Hector. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
description This is the second article of a series devoted to European Extremely Large Telescope (E-ELT) site characterization. In this article we present the main properties of the parameters involved in high angular resolution observations from the data collected in the site testing campaign of the E-ELT during the design study (DS) phase. Observations were made in 2008 and 2009, in the four sites selected to shelter the future E-ELT (characterized under the ELT-DS contract): Aklim mountain in Morocco, Observatorio del Roque de los Muchachos (ORM) in Spain, Macón range in Argentina, and Cerro Ventarrones in Chile. The same techniques, instruments, and acquisition procedures were taken on each site. A multiple aperture scintillation sensor (MASS) and a differential image motion monitor (DIMM) were installed at each site. Global statistics of the integrated seeing, the free atmosphere seeing, the boundary layer seeing, and the isoplanatic angle were studied for each site, and the results are presented here. In order to estimate other important parameters, such as the coherence time of the wavefront and the overall parameter “coherence étendue,” additional information of vertical profiles of the wind speed was needed. Data were retrieved from the National Oceanic and Atmospheric Administration (NOAA) archive. Ground wind speed was measured by automatic weather stations (AWS). More aspects of the turbulence parameters, such as their seasonal trend, their nightly evolution, and their temporal stability, were also obtained and analyzed.
publishDate 2012
dc.date.none.fl_str_mv 2012-08
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/11336/272710
Vázquez Ramió, Héctor; Vernin, Jean; Muñoz Tuñon, Casiana; Sarazin, Marc; Varela, Antonia M.; et al.; European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters; University of Chicago Press; Publications of the Astronomical Society of the Pacific; 124; 918; 8-2012; 868-884
0004-6280
CONICET Digital
CONICET
url http://hdl.handle.net/11336/272710
identifier_str_mv Vázquez Ramió, Héctor; Vernin, Jean; Muñoz Tuñon, Casiana; Sarazin, Marc; Varela, Antonia M.; et al.; European Extremely Large Telescope Site Characterization. II. High Angular Resolution Parameters; University of Chicago Press; Publications of the Astronomical Society of the Pacific; 124; 918; 8-2012; 868-884
0004-6280
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://iopscience.iop.org/article/10.1086/667599
info:eu-repo/semantics/altIdentifier/doi/10.1086/667599
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
dc.publisher.none.fl_str_mv University of Chicago Press
publisher.none.fl_str_mv University of Chicago Press
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
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