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dc.contributor.authorColodro Conde, Carlos 
dc.contributor.authorToledo Moreo, Rafael 
dc.contributor.authorFernández Valdivia Juan José es_ES
dc.contributor.authorLópez López, Roberto es_ES
dc.contributor.authorOscoz Abad, Alejandro es_ES
dc.contributor.authorRebolo López, Rafael es_ES
dc.contributor.authorFemenia, Bruno es_ES
dc.contributor.authorLabadie, Lucas es_ES
dc.contributor.authorMackay, Craig es_ES
dc.contributor.authorPérez Garrido, Antonio es_ES
dc.contributor.authorPuga Antolín, Marta es_ES
dc.contributor.authorRodríguez Coira, Gustavo es_ES
dc.contributor.authorRodríguez Ramos, Luis Fernando es_ES
dc.contributor.authorRodríguez Ramos, José Manuel es_ES
dc.contributor.authorVillo Pérez, Isidro es_ES
dc.contributor.authorKing, David L. es_Es
dc.contributor.authorToledo Moreo, Rafael es_Es
dc.date.accessioned2018-02-27T11:28:57Z
dc.date.available2018-02-27T11:28:57Z
dc.date.issued2017-06
dc.identifier.citationCOLODRO CONCE, Carlos et al. Laboratory and telescope demonstration of the TP3-WFS for the adaptive optics segment of AOLI. In: Monthly Notices of the Royal Astronomical Society 467.3 (Jun. 2017), pp. 2855–2868.es_ES
dc.identifier.issn0035-8711
dc.description.abstractAOLI (Adaptive Optics Lucky Imager) is a state-of-art instrument that combines adaptive optics (AO) and lucky imaging (LI) with the objective of obtaining diffraction limited images in visible wavelength at mid- and big-size ground-based telescopes. The key innovation of AOLI is the development and use of the new TP3-WFS (Two Pupil Plane PositionsWavefront Sensor). The TP3-WFS, working in visible band, represents an advance over classical wavefront sensors such as the Shack-Hartmann WFS (SH-WFS) because it can theoretically use fainter natural reference stars, which would ultimately provide better sky coverages to AO instruments using this newer sensor. This paper describes the software, algorithms and procedures that enabled AOLI to become the first astronomical instrument performing real-time adaptive optics corrections in a telescope with this new type of WFS, including the first control-related results at the William Herschel Telescope (WHT)es_ES
dc.description.sponsorshipThis work was supported by the Spanish Ministry of Economy under the projects AYA2011-29024, ESP2014-56869-C2-2-P, ESP2015-69020-C2-2-R and DPI2015-66458-C2-2-R, by project 15345/PI/10 from the Fundación Séneca, by the Spanish Ministry of Education under the grant FPU12/05573, by project ST/K002368/1 from the Science and Technology Facilities Council and by ERDF funds from the European Commission. The results presented in this paper are based on observations made with the William Herschel Telescope operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. Special thanks go to Lara Monteagudo and Marcos Pellejero for their timely contributions.es_ES
dc.formatapplication/pdfes_ES
dc.language.isoenges_ES
dc.publisherBlackwelles_ES
dc.relationContributions to technology and techniques for ground-based and space-based astronomy synthesis of EDAC codecs, AOLI and COELI.
dc.relation.urihttp://hdl.handle.net/10317/6672
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España*
dc.rights© Copyright 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.titleLaboratory and telescope demonstration of the TP3-WFS for the adaptive optics segment of AOLIes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.subject.otherArquitectura y Tecnología de Computadorases_ES
dc.subjectInstrumentation: adaptive opticses_ES
dc.subjectInstrumentation: high angular resolutiones_ES
dc.identifier.urihttp://hdl.handle.net/10317/6674
dc.peerreviewSies_ES
dc.identifier.doi10.1093/mnras/stx262
dc.identifier.urlhttps://academic.oup.com/mnras/article-abstract/467/3/2855/2966871?redirectedFrom=fulltext
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.type.versioninfo:eu-repo/semantics/submittedVersiones_ES
dc.relation.projectIDAYA2011-29024es_ES
dc.relation.projectIDESP2014-56869- C2-2-P
dc.relation.projectIDESP2015-69020-C2-2-Res_ES
dc.relation.projectIDDPI2015-66458-C2-2-Res_ES
dc.relation.projectID15345/PI/10es_ES
dc.relation.projectIDFPU12/05573es_ES
dc.relation.projectIDST/K002368/1es_ES
dc.subject.unesco2203 Electrónicaes_ES
dc.contributor.funderMinisterio de Economía, Industria y Competitividades_ES
dc.contributor.funderMinisterio de Educación, Cultura y Deportees_ES
dc.contributor.funderFundación Senecaes_ES
dc.contributor.funderInstituto de Astrofísica de Canariases_ES


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