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dc.contributor.author
Pareschi, G.  
dc.contributor.author
Medina, Maria Clementina  
dc.contributor.author
CTA Consortium  
dc.date.available
2016-04-14T19:50:12Z  
dc.date.issued
2013-09  
dc.identifier.citation
Pareschi, G.; Medina, Maria Clementina; CTA Consortium; Status of the technologies for the production of the Cherenkov Telescope Array (CTA) mirrors; SPIE; Spie Proceedings; 8861; 9-2013; 886103-886103  
dc.identifier.issn
0277-786X  
dc.identifier.uri
http://hdl.handle.net/11336/5206  
dc.description.abstract
The Cherenkov Telescope Array (CTA) is the next generation very high-energy gamma-ray observatory, with at least 10 times higher sensitivity than current instruments. CTA will comprise several tens of Imaging Atmospheric Cherenkov Telescopes (IACTs) operated in array-mode and divided into three size classes: large, medium and small telescopes. The total reflective surface could be up to 10,000 m2 requiring unprecedented technological efforts. The properties of the reflector directly influence the telescope performance and thus constitute a fundamental ingredient to improve and maintain the sensitivity. The R&D status of lightweight, reliable and cost-effective mirror facets for the CTA telescope reflectors for the different classes of telescopes is reviewed in this paper.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
SPIE  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
CHERENKOV TELESCOPE ARRAY  
dc.subject
CHERENKOV TELESCOPES  
dc.subject
MIRRORS  
dc.subject
REFLECTING COATINGS  
dc.subject.classification
Astronomía  
dc.subject.classification
Ciencias Físicas  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
Status of the technologies for the production of the Cherenkov Telescope Array (CTA) mirrors  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2016-05-06 15:52:43.262787-03  
dc.journal.volume
8861  
dc.journal.pagination
886103-886103  
dc.journal.pais
Estados Unidos  
dc.journal.ciudad
Bellingham  
dc.conicet.avisoEditorial
Copyright [2013] Society of Photo Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic electronic or print reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.  
dc.description.fil
Fil: Pareschi, G.. INAF/Brera Astronomical Observatory; Italia  
dc.description.fil
Fil: Medina, Maria Clementina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina  
dc.description.fil
Fil: CTA Consortium. No especifíca;  
dc.journal.title
Spie Proceedings  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://arxiv.org/abs/1310.1713  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1744847  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1117/12.2025476