Introducing the CTA concept
dc.contributor.author | Antoranz Canales, Pedro | |
dc.contributor.author | Barrio Uña, Juan Abel | |
dc.contributor.author | Bernardino Santos, Teodoro | |
dc.contributor.author | Contreras González, José Luis | |
dc.contributor.author | Fonseca González, Mª Victoria | |
dc.contributor.author | Hassan, Tarek | |
dc.contributor.author | López Moya, Marcos | |
dc.contributor.author | Mirabal Barrios, Néstor | |
dc.contributor.author | Miranda Pantoja, José Miguel | |
dc.contributor.author | Satalecka, Konstanzja | |
dc.contributor.author | Scapin, Valeria | |
dc.contributor.author | Tejedor Álvarez, Luis Ángel | |
dc.contributor.author | Yebras Rivera, José Manuel | |
dc.date.accessioned | 2023-06-19T13:23:29Z | |
dc.date.available | 2023-06-19T13:23:29Z | |
dc.date.issued | 2013-03 | |
dc.description | © 2013 Elsevier BV. | |
dc.description.abstract | The Cherenkov Telescope Array (CTA) is a new observatory for very high-energy (VHE) gamma rays. CTA has ambitions science goals, for which it is necessary to achieve full-sky coverage, to improve the sensitivity by about an order of magnitude, to span about four decades of energy, from a few tens of GeV to above 100 TeV with enhanced angular and energy resolutions over existing VHE gamma-ray observatories. An international collaboration has formed with more than 1000 members from 27 countries in Europe, Asia, Africa and North and South America. In 2010 the CTA Consortium completed a Design Study and started a three-year Preparatory Phase which leads to production readiness of CTA in 2014. In this paper we introduce the science goals and the concept of CTA, and provide an overview of the project. (C) 2013 Elsevier B.V. All rights reserved. | |
dc.description.department | Depto. de Estructura de la Materia, Física Térmica y Electrónica | |
dc.description.faculty | Fac. de Ciencias Físicas | |
dc.description.refereed | TRUE | |
dc.description.status | pub | |
dc.eprint.id | https://eprints.ucm.es/id/eprint/24791 | |
dc.identifier.citation | [1] A.M. Hillas, Evolution of ground-based gamma-ray astronomy from the early days to the Cherenkov telescope arrays, Astropart. Phys. (2012), http:// x.doi.org/10.1016/j.astropartphys.2012.06.002. [2] F. Aharonian et al., HESS Collaboration, A&A 457 (2006) 899, ttp://www.mpihd.mpg.de/hfm/HESS/pages/about/telescopes>. [3] MAGIC. <http://magic.mppmu.mpg.de>. [4] VERITAS. <http://veritas.sao.arizona.edu>. [5] W.B. Atwood et al., ApJ 697 (2009) 1071, ttp://dx.doi.org/10.1088/0004-637X/697/2/1071 http://fermi.gsfc.nasa.gov>. [6] M. Tavani et al., NIM A588 (2008) 52. [7] Milagro. <http://www.lanl.gov/milagro>. [8] Tibet AS Gamma. <http://www.icrr.utokyo.ac.jp/em/index.html>. [9] G. Aielli et al., Nucl. Instrum. Methods Phys. Res. A. 562 (2006) 92. <http://argo.na.infn.it>. [10] J.A. Hinton, W. Hofmann, Ann. Rev. Astronom. Astrophys. 47 (2009) 523. [11] F.A. Aharonian et al., Rep. Prog. Phys. 71 (2008)096901. [12] M. Actis et al., CTA Consortium, Exp. Astronom. 32 (2011) 193–316. http://www.cta-observatory.org. [13] F. Aharonian et al., HESS Collaboration, ApJ 636 (2006) 777–797, http://dx.doi.org/10.1086/498013. <arXiv:astro-ph/0510397>. [14] HAWC, <http://hawc.umd.edu>. [15] J.A. Hinton, New J. Phys. 11 (2009) 055005. [16] G. Fontaine, Towards a Major Atmospheric Cherenkov Detector, Ed. Frontiers 1992. [17] M. Martínez, J. Phys. Conf. Ser. 171 (2009) 012013. [18] A.A. Abdo et al., Science 327 (2010) 1103. [19] M. Tavani et al., ApJ Lett. 710 (2010) L151; A. Giuliani et al., ApJ Lett. 742 (2011) L30. [20] F. Acero et al., Gamma-ray signatures of cosmic ray acceleration, propagation, and confinement in the era of CTA, Astropart. Phys. (2012), http://dx.doi.org/10.1016/j.astropartphys.2012.05.024. [21] H. Sol et al., Active Galactic Nuclei under the scrutiny of CTA, Astropart. Phys. (2012). this issue. [22] D. Mazin et al., Potential of EBL and cosmology studies with the Cherenkov Telescope Array, Astropart. Phys. (2012). [23] M. Doro et al., Dark matter and fundamental physics with the Cherenkov Telescope Array, Astropart. Phys. (2012), http://dx.doi.org/10.1016/j.astropartphys.2012.08.002. [24] D. Dravins et al., Optical intensity interferometry with the Cherenkov Telescope Array, Astropart. Phys. (2012), http://dx.doi.org/10.1016/j.astropartphys.2012.04.017. [25] S. Funk, J.A. Hinton, Comparison of Fermi-LAT and CTA in the region between 10–100 GeV, Astropart. Phys. (2012), http://dx.doi.org/10.1016/j.astropartphys.2012.05.018. [26] E. de Oña-Wilhelmi et al., Prospects for observations of pulsars and pulsar wind nebulae with CTA, Astropart. Phys. (2012), http://dx.doi.org/10.1016/j.astropartphys.2012.08.009. [27] J.M. Paredes et al., Binaries with the eyes of CTA, Astropart. Phys. (2012), http://dx.doi.org/10.1016/j.astropartphys.2012.09.004. [28] S. Inoue et al., Gamma-Ray burst science in the era of the Cherenkov Telescope Array, Astropart. Phys. (2012). this issue. [29] G. Dubus et al., Surveys with the Cherenkov telescope array, Astropart. Phys. (2012), http://dx.doi.org/10.1016/j.astropartphys.2012.05.020. [30] T. Bretz et al., FACT Collaboration, FACT – The First G-APD Cherenkov Telescope (first results), in: Proceedings of 5th International Symposium on Gamma-Ray Astronomy, Heidelberg, 2012. [31] K. Bernlöhr et al., Monte Carlo design studies for the Cherenkov Telescope Array, Astropart. Phys. (2012), http://dx.doi.org/10.1016/j.astropartphys.2012.10.002. [32] Alma, <http://www.almaobservatory.org>. [33] E-ELT, <http://www.eso.org/public/teles-instr/e-elt.html>. [34] SKA, <http://www.skatelescope.org>. [35] LSST, <http://www.lsst.org>. [36] ESFRI Roadmap, <ftp://ftp.cordis.europa.eu/pub/esfri/docs/esfriroadmapupdate2008.pdf>. [37] ASPERA Roadmap, <http://www.aspera-eu.org/images/stories/roadmap/asperaroadmap.pdf>. [38] ASTRONET Roadmap, <http://www.astronet-eu.org/IMG/pdf/Astronet-Book.pdf>. [39] Decadal Survey, <http://sites.nationalacademies.org/bpa/BPA049810>. | |
dc.identifier.doi | 10.1016/j.astropartphys.2013.01.007 | |
dc.identifier.issn | 0927-6505 | |
dc.identifier.officialurl | http://dx.doi.org/10.1016/j.astropartphys.2013.01.007 | |
dc.identifier.relatedurl | http://www.sciencedirect.com | |
dc.identifier.uri | https://hdl.handle.net/20.500.14352/33495 | |
dc.issue.number | 17SI | |
dc.journal.title | Astroparticle Physics | |
dc.language.iso | eng | |
dc.page.final | 18 | |
dc.page.initial | 3 | |
dc.publisher | Elsevier Science BV | |
dc.rights.accessRights | restricted access | |
dc.subject.cdu | 537 | |
dc.subject.cdu | 539.1 | |
dc.subject.keyword | Supernova Ramnant W44 | |
dc.subject.keyword | Telescope | |
dc.subject.keyword | Astronomy | |
dc.subject.keyword | Emission | |
dc.subject.keyword | Mission | |
dc.subject.keyword | Hess. | |
dc.subject.ucm | Electricidad | |
dc.subject.ucm | Electrónica (Física) | |
dc.subject.ucm | Física nuclear | |
dc.subject.unesco | 2202.03 Electricidad | |
dc.subject.unesco | 2207 Física Atómica y Nuclear | |
dc.title | Introducing the CTA concept | |
dc.type | journal article | |
dc.volume.number | 43 | |
dspace.entity.type | Publication | |
relation.isAuthorOfPublication | 6bc87e5f-9b77-4982-b112-0d4f8aa128d0 | |
relation.isAuthorOfPublication | 11e5fd8b-1a86-4f8d-85c6-135541232be4 | |
relation.isAuthorOfPublication | 6a14529e-a65e-4709-9bc1-61f9429841c1 | |
relation.isAuthorOfPublication | 8b5d96d7-bd11-4ee4-87d0-258a1e077e26 | |
relation.isAuthorOfPublication | 328f9716-2012-44f9-aacc-ef8d48782a77 | |
relation.isAuthorOfPublication | 25cc9bbf-c7d1-49ea-a4ea-eab74ab3c838 | |
relation.isAuthorOfPublication.latestForDiscovery | 6bc87e5f-9b77-4982-b112-0d4f8aa128d0 |
Download
Original bundle
1 - 1 of 1
No Thumbnail Available
- Name:
- MirandaJM117.pdf
- Size:
- 1.82 MB
- Format:
- Adobe Portable Document Format