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The large size telescope of the Cherenkov Telescope array

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dc.contributor.authorBarrio Uña, Juan Abel
dc.contributor.authorContreras González, José Luis
dc.contributor.authorLópez Moya, Marcos
dc.contributor.authorMiranda Pantoja, José Miguel
dc.contributor.authorTejedor Álvarez, Luis Ángel
dc.date.accessioned2023-06-19T14:55:12Z
dc.date.available2023-06-19T14:55:12Z
dc.date.issued2014
dc.description© 2014 SPIE. Conference on Ground-Based and Airborne Telescopes V (2014. Montreal-Canada). Artículo firmado por 131 autores. We gratefully acknowledge financial support from the following agencies and organizations: Ministerio de Ciencia, Tecnología e Innovación Productiva (MinCyT), Comisión Nacional de Energía Atómica (CNEA), Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Argentina; State Committee of Science of Armenia, Armenia; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Fundação de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ), Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP), Brasil; Croatian Science Foundation, Croatia; Ministry of Education, Youth and Sports, MEYS LE13012, 7AMB12AR013, Czech Republic; Ministry of Higher Education and Research, CNRSINSU and CNRS-IN2P3, CEA-Irfu, ANR, Regional Council Ile de France, Labex ENIGMASS, OSUG2020 and OCEVU, France; Max Planck Society, BMBF, DESY, Helmholtz Association, Germany; Department of Atomic Energy, Department of Science and Technology, India; Istituto Nazionale di Astrofisica (INAF), MIUR, Italy; Istituto Nazionale di Fisica Nucleare (INFN), Italy; ICRR, University of Tokyo, JSPS, Japan; Netherlands Research School for Astronomy (NOVA), Netherlands Organization for Scientific Research (NWO), Netherlands; The Bergen Research Foundation, Norway; Ministry of Science and Higher Education, the National Centre for Research and Development and the National Science Centre, Poland; MINECO support through the National R+D+I, CDTI funding plans and the CPAN and MultiDark Consolider-Ingenio 2010 programme, Spain; Swedish Research Council, Royal Swedish Academy of Sciences, Sweden; Swiss National Science Foundation (SNSF), Ernest Boninchi Foundation, Switzerland; Durham University, Leverhulme Trust, Liverpool University, University of Leicester, University of Oxford, Royal Society, Science and Technologies Facilities Council, UK; U.S. National Science Foundation, U.S. Department of Energy, Argonne National Laboratory, Barnard College, University of California, University of Chicago, Columbia University, Georgia Institute of Technology, Institute for Nuclear and Particle Astrophysics (INPACMRPI program), Iowa State University, Washington University McDonnell Center for the Space Sciences, USA. The research leading to these results has received funding from the European Union’s Seventh Framework Programme (FP7/2007-2013) under grant agreement nº 262053.
dc.description.abstractThe Cherenkov Telescope Array (CTA) project aims to implement the world’s largest next generation of Very High Energy gamma-ray Imaging Atmospheric Cherenkov Telescopes devoted to the observation from a few tens of GeV to more than 100 TeV. To view the whole sky, two CTA sites are foreseen, one for each hemisphere. The sensitivity at the lowest energy range will be dominated by four Large Size Telescopes, LSTs, located at the center of each array and designed to achieve observations of high red-shift objects with the threshold energy of 20 GeV. The LST is optimized also for transient low energy sources, such as Gamma Ray Bursts (GRB), which require fast repositioning of the telescope. The overall design and the development status of the first LST telescope will be discussed.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUnión Europea. FP7
dc.description.sponsorshipMinisterio de Ciencia, Tecnología e Innovación Productiva (MinCyT), Argentina
dc.description.sponsorshipComisión Nacional de Energía Atómica (CNEA), Argentina
dc.description.sponsorshipConsejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Argentina
dc.description.sponsorshipState Committee of Science of Armenia
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Brasil
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ)
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipCroatian Science Foundation
dc.description.sponsorshipMinistry of Education, Czech Republic
dc.description.sponsorshipMinistry of Higher Education and Research, Czech Republic
dc.description.sponsorshipMinistry of Higher Education and Research, FRance
dc.description.sponsorshipRegional Council Ile de France
dc.description.sponsorshipMax Planck Society, Germany
dc.description.sponsorshipBMBF, Germany
dc.description.sponsorshipDESY, Germany
dc.description.sponsorshipHelmholtz Association, Germany
dc.description.sponsorshipDepartment of Atomic Energy, India
dc.description.sponsorshipDepartment of Science and Technology, India
dc.description.sponsorshipIstituto Nazionale di Astrofisica (INAF), Italy
dc.description.sponsorshipMIUR, Italy
dc.description.sponsorshipIstituto Nazionale di Fisica Nucleare (INFN), Italy
dc.description.sponsorshipICRR, Japan
dc.description.sponsorshipUniversity of Tokyo
dc.description.sponsorshipJSPS, Japan
dc.description.sponsorshipNetherlands Research School for Astronomy (NOVA)
dc.description.sponsorshipNetherlands Organization for Scientific Research (NWO)
dc.description.sponsorshipThe Bergen Research Foundation, Norway
dc.description.sponsorshipMinistry of Science and Higher Education, Poland
dc.description.sponsorshipNational Centre for Research and Development and the National Science Centre, Poland
dc.description.sponsorshipMINECO support through the National R+D+I
dc.description.sponsorshipCDTI, Spain
dc.description.sponsorshipCPAN, Spain
dc.description.sponsorshipConsolider-Ingenio 2010 programme, Spain
dc.description.sponsorshipSwedish Research Council
dc.description.sponsorshipRoyal Swedish Academy of Sciences
dc.description.sponsorshipSwiss National Science Foundation (SNSF)
dc.description.sponsorshipErnest Boninchi Foundation, Switzerland
dc.description.sponsorshipDurham University, UK
dc.description.sponsorshipLeverhulme Trust, UK
dc.description.sponsorshipLiverpool University
dc.description.sponsorshipUniversity of Leicester
dc.description.sponsorshipUniversity of Oxford
dc.description.sponsorshipRoyal Society, Science and Technologies Facilities Council, UK
dc.description.sponsorshipU.S. National Science Foundation
dc.description.sponsorshipU.S. Department of Energy
dc.description.sponsorshipArgonne National Laboratory, USA
dc.description.sponsorshipBarnard College, USA
dc.description.sponsorshipUniversity of California
dc.description.sponsorshipUniversity of Chicago
dc.description.sponsorshipColumbia University
dc.description.sponsorshipGeorgia Institute of Technology
dc.description.sponsorshipInstitute for Nuclear and Particle Astrophysics (INPACMRPI program), USA
dc.description.sponsorshipIowa State University
dc.description.sponsorshipWashington University McDonnell Center for the Space Sciences, USA
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/31319
dc.identifier.doi10.1117/12.2054605
dc.identifier.issn0277-786X
dc.identifier.officialurlhttp://dx.doi.org/10.1117/12.2054605
dc.identifier.relatedurlhttp://proceedings.spiedigitallibrary.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/34774
dc.journal.titleProceedings of SPIE
dc.language.isoeng
dc.publisherSpie-Int. Soc. Optical Engineering
dc.relation.projectIDFP7/2007-2013 (262053)
dc.relation.projectIDLE13012
dc.relation.projectID7AMB12AR013
dc.relation.projectIDCNRSINSU
dc.relation.projectIDCNRS-IN2P3
dc.relation.projectIDCEA-Irfu
dc.relation.projectIDANR
dc.relation.projectIDLabex ENIGMASS
dc.relation.projectIDOSUG2020
dc.relation.projectIDOCEVU
dc.rights.accessRightsopen access
dc.subject.cdu537
dc.subject.cdu539.1
dc.subject.keywordImaging atmospheric Cherenkov telescope
dc.subject.keywordCTA
dc.subject.keywordGamma-rays.
dc.subject.ucmElectricidad
dc.subject.ucmElectrónica (Física)
dc.subject.ucmFísica nuclear
dc.subject.unesco2202.03 Electricidad
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleThe large size telescope of the Cherenkov Telescope array
dc.typejournal article
dc.volume.number9145
dcterms.references[1] The Cherenkov Telescope Array, http://www.cta-observatory.org/. [2] Cortina J., et al., "The Large Size Telescope, a 23 m diameter Cherenkov telescope for the Cherenkov Telescope Array made of high strength, low weight carbon fiber reinforced plastic tubes," Proc. ICRC, (2013). [3] Vernani D., et al., "Glass mirrors by cold slumping to cover 100 m2 of the MAGIC II Cherenkov telescope reflecting surface," Proc. SPIE 7018, (2008). [4] Lamanna G., et al., "Large Size Telescope camera support structures for the Cherenkov Telescope Array," Proc. ICRC, (2013). [5] Delgado C., et al., Mechanics and cooling system for the camera of the Large Size Telescopes of the Cherenkov Telescope Array (CTA)," Proc ICRC, (2013). [6] Yamamoto T., "Development of the Camera for the Large Size Telescopes of the Cherenkov Telescope Array," Proc. SPIE, (2014). [7] Okumura A., https://github.com/akira-okumura/ROBAST. [8] Sanuy A. et al., "Wideband (500 MHz) 16 bit dynamic range current mode PreAmplifier for the CTA cameras (PACTA)," JINST, 7, (2012). [9] Tejedor L.A., et al., "An Analog Trigger System for Atmospheric Cherenkov Telescope Arrays," IEEE Transactions on Nuclear Science, Vol. 60 Issue 3, (2013). [10]Sulanke K.H., et al., " A Digital Camera Trigger for the Cherenkov Telescope Array," Proc. ICRC, (2013). [11]Ritt S., Dinapoli R., Hartmann U., " Application of the DRS chip for fast waveform digitizing," Nuclear Instruments and Methods A, Vol. 623, (2010). [12]Kubo H., Paoletti R., et al., "Development of the Photomultiplier-Tube Readout System for the CTA Large Size Telescope," Proc. ICRC, (2013).
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