Design of a 7m Davies-Cotton Cherenkov telescope mount for the high energy section of the Cherenkov Telescope Array

The Cherenkov Telescope Array is the next generation ground-based observatory for the study of very-high-energy gamma-rays. It will provide an order of magnitude more sensitivity and greater angular resolution than present systems as well as an increased energy range (20 GeV to 300 TeV). For the hig...

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Detalles Bibliográficos
Autores principales: Rovero, Adrian Carlos, Ringegni, Pablo Lorenzo, Vallejo, Gonzalo, Supanitsky, Alberto Daniel, Actis, Marcos Daniel, Botani, Asdrubal, Ochoa, Ignacio, Hughes, G.
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2013
Materias:
CTA
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/102592
https://ri.conicet.gov.ar/11336/17063
https://link.springer.com/article/10.1007%2Fs10686-013-9333-6
Aporte de:
id I19-R120-10915-102592
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Física
CTA
Gamma-rays
Imaging atmospheric cherenkov telescope
Telescope optics
Telescope aberrations
Telescope mechanical moun
spellingShingle Ciencias Astronómicas
Física
CTA
Gamma-rays
Imaging atmospheric cherenkov telescope
Telescope optics
Telescope aberrations
Telescope mechanical moun
Rovero, Adrian Carlos
Ringegni, Pablo Lorenzo
Vallejo, Gonzalo
Supanitsky, Alberto Daniel
Actis, Marcos Daniel
Botani, Asdrubal
Ochoa, Ignacio
Hughes, G.
Design of a 7m Davies-Cotton Cherenkov telescope mount for the high energy section of the Cherenkov Telescope Array
topic_facet Ciencias Astronómicas
Física
CTA
Gamma-rays
Imaging atmospheric cherenkov telescope
Telescope optics
Telescope aberrations
Telescope mechanical moun
description The Cherenkov Telescope Array is the next generation ground-based observatory for the study of very-high-energy gamma-rays. It will provide an order of magnitude more sensitivity and greater angular resolution than present systems as well as an increased energy range (20 GeV to 300 TeV). For the high energy portion of this range, a relatively large area has to be covered by the array. For this, the construction of ~7 m diameter Cherenkov telescopes is an option under study. We have proposed an innovative design of a Davies-Cotton mount for such a telescope, within Cherenkov Telescope Array specifications, and evaluated its mechanical and optical performance. The mount is a reticulated-type structure with steel tubes and tensioned wires, designed in three main parts to be assembled on site. In this work we show the structural characteristics of the mount and the optical aberrations at the focal plane for three options of mirror facet size caused by mount deformations due to wind and gravity.
format Articulo
Preprint
author Rovero, Adrian Carlos
Ringegni, Pablo Lorenzo
Vallejo, Gonzalo
Supanitsky, Alberto Daniel
Actis, Marcos Daniel
Botani, Asdrubal
Ochoa, Ignacio
Hughes, G.
author_facet Rovero, Adrian Carlos
Ringegni, Pablo Lorenzo
Vallejo, Gonzalo
Supanitsky, Alberto Daniel
Actis, Marcos Daniel
Botani, Asdrubal
Ochoa, Ignacio
Hughes, G.
author_sort Rovero, Adrian Carlos
title Design of a 7m Davies-Cotton Cherenkov telescope mount for the high energy section of the Cherenkov Telescope Array
title_short Design of a 7m Davies-Cotton Cherenkov telescope mount for the high energy section of the Cherenkov Telescope Array
title_full Design of a 7m Davies-Cotton Cherenkov telescope mount for the high energy section of the Cherenkov Telescope Array
title_fullStr Design of a 7m Davies-Cotton Cherenkov telescope mount for the high energy section of the Cherenkov Telescope Array
title_full_unstemmed Design of a 7m Davies-Cotton Cherenkov telescope mount for the high energy section of the Cherenkov Telescope Array
title_sort design of a 7m davies-cotton cherenkov telescope mount for the high energy section of the cherenkov telescope array
publishDate 2013
url http://sedici.unlp.edu.ar/handle/10915/102592
https://ri.conicet.gov.ar/11336/17063
https://link.springer.com/article/10.1007%2Fs10686-013-9333-6
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