Introducing the CTA concept

B. S. Acharya; M. Actis; T. Aghajani; G. Agnetta; J. Aguilar; F. Aharonian; M. Ajello; A. Akhperjanian; M. Alcubierre; J. Aleksić; R. Alfaro; E. Aliu; A. J. Allafort; D. Allan; I. Allekotte; E. Amato; J. Anderson; E. O. Anguner; L. A. Antonelli; P. Antoranz; A. Aravantinos; T. Arlen; T. Armstrong; H. Arnaldi; L. Arrabito; K. Asano; T. Ashton; H. G. Asorey; Y. Awane; H. Baba; A. Babic; N. Baby; J. Bahr; A. Bais; C. Baixeras; S. Bajtlik; M. Balbo; D. Balis; C. Balkowski; A. Bamba; R. Bandiera; A. Barber; C. Barbier; M. Barcelo; A. Barnacka; J. Barnstedt; U. De AlmeidaBarres; J. A. Barrio; A. Basili; S. Basso; D. Bastieri; C. Bauer; A. Baushev; J. Becerra; Y. Becherini; K. C. Bechtol; J. Becker Tjus; V. Beckmann; W. Bednarek; B. Behera; M. Belluso; W. Benbow; J. Berdugo; K. Berger; F. Bernard; T. Bernardino; K. Bernlohr; N. Bhat; S. Bhattacharyya; C. Bigongiari; A. Biland; S. Billotta; T. Bird; E. Birsin; E. Bissaldi; J. Biteau; M. Bitossi; S. Blake; O. Blanch Bigas; P. Blasi; A. Bobkov; V. Boccone; M. Boettcher; L. Bogacz; J. Bogart; M. Bogdan; C. Boisson; J. Boix Gargallo; J. Bolmont; G. Bonanno; A. Bonardi; T. Bonev; P. Bonifacio; G. Bonnoli; P. Bordas; A. Borgland; J. Borkowski; R. Bose; O. Botner; A. Bottani

doi:10.1016/j.astropartphys.2013.01.007

Introducing the CTA concept

B. S. Acharya, M. Actis, T. Aghajani, G. Agnetta, J. Aguilar, F. Aharonian, M. Ajello, A. Akhperjanian, M. Alcubierre, J. Aleksić, R. Alfaro, E. Aliu, A. J. Allafort, D. Allan, I. Allekotte, E. Amato, J. Anderson, E. O. Anguner, L. A. Antonelli, P. AntoranzA. Aravantinos, T. Arlen, T. Armstrong, H. Arnaldi, L. Arrabito, K. Asano, T. Ashton, H. G. Asorey, Y. Awane, H. Baba, A. Babic, N. Baby, J. Bahr, A. Bais, C. Baixeras, S. Bajtlik, M. Balbo, D. Balis, C. Balkowski, A. Bamba, R. Bandiera, A. Barber, C. Barbier, M. Barcelo, A. Barnacka, J. Barnstedt, U. De AlmeidaBarres, J. A. Barrio, A. Basili, S. Basso, D. Bastieri, C. Bauer, A. Baushev, J. Becerra, Y. Becherini, K. C. Bechtol, J. Becker Tjus, V. Beckmann, W. Bednarek, B. Behera, M. Belluso, W. Benbow, J. Berdugo, K. Berger, F. Bernard, T. Bernardino, K. Bernlohr, N. Bhat, S. Bhattacharyya, C. Bigongiari, A. Biland, S. Billotta, T. Bird, E. Birsin, E. Bissaldi, J. Biteau, M. Bitossi, S. Blake, O. Blanch Bigas, P. Blasi, A. Bobkov, V. Boccone, M. Boettcher, L. Bogacz, J. Bogart, M. Bogdan, C. Boisson, J. Boix Gargallo, J. Bolmont, G. Bonanno, A. Bonardi, T. Bonev, P. Bonifacio, G. Bonnoli, P. Bordas, A. Borgland, J. Borkowski, R. Bose, O. Botner, A. Bottani

Department of Physics

Research output: Contribution to journal › Article › Research › peer-review

566 Citations (Scopus)

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. © 2013 Elsevier B.V. All rights reserved.

Original language	English
Pages (from-to)	3-18
Journal	Astroparticle Physics
Volume	43
DOIs	https://doi.org/10.1016/j.astropartphys.2013.01.007
Publication status	Published - 1 Jan 2013

Keywords

Air showers
Cherenkov Telescopes
TeV gamma-ray astronomy

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10.1016/j.astropartphys.2013.01.007

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Acharya, B. S., Actis, M., Aghajani, T., Agnetta, G., Aguilar, J., Aharonian, F., Ajello, M., Akhperjanian, A., Alcubierre, M., Aleksić, J., Alfaro, R., Aliu, E., Allafort, A. J., Allan, D., Allekotte, I., Amato, E., Anderson, J., Anguner, E. O., Antonelli, L. A., ... Bottani, A. (2013). Introducing the CTA concept. Astroparticle Physics, 43, 3-18. https://doi.org/10.1016/j.astropartphys.2013.01.007

Acharya, B. S. ; Actis, M. ; Aghajani, T. ; Agnetta, G. ; Aguilar, J. ; Aharonian, F. ; Ajello, M. ; Akhperjanian, A. ; Alcubierre, M. ; Aleksić, J. ; Alfaro, R. ; Aliu, E. ; Allafort, A. J. ; Allan, D. ; Allekotte, I. ; Amato, E. ; Anderson, J. ; Anguner, E. O. ; Antonelli, L. A. ; Antoranz, P. ; Aravantinos, A. ; Arlen, T. ; Armstrong, T. ; Arnaldi, H. ; Arrabito, L. ; Asano, K. ; Ashton, T. ; Asorey, H. G. ; Awane, Y. ; Baba, H. ; Babic, A. ; Baby, N. ; Bahr, J. ; Bais, A. ; Baixeras, C. ; Bajtlik, S. ; Balbo, M. ; Balis, D. ; Balkowski, C. ; Bamba, A. ; Bandiera, R. ; Barber, A. ; Barbier, C. ; Barcelo, M. ; Barnacka, A. ; Barnstedt, J. ; De AlmeidaBarres, U. ; Barrio, J. A. ; Basili, A. ; Basso, S. ; Bastieri, D. ; Bauer, C. ; Baushev, A. ; Becerra, J. ; Becherini, Y. ; Bechtol, K. C. ; Becker Tjus, J. ; Beckmann, V. ; Bednarek, W. ; Behera, B. ; Belluso, M. ; Benbow, W. ; Berdugo, J. ; Berger, K. ; Bernard, F. ; Bernardino, T. ; Bernlohr, K. ; Bhat, N. ; Bhattacharyya, S. ; Bigongiari, C. ; Biland, A. ; Billotta, S. ; Bird, T. ; Birsin, E. ; Bissaldi, E. ; Biteau, J. ; Bitossi, M. ; Blake, S. ; Blanch Bigas, O. ; Blasi, P. ; Bobkov, A. ; Boccone, V. ; Boettcher, M. ; Bogacz, L. ; Bogart, J. ; Bogdan, M. ; Boisson, C. ; Boix Gargallo, J. ; Bolmont, J. ; Bonanno, G. ; Bonardi, A. ; Bonev, T. ; Bonifacio, P. ; Bonnoli, G. ; Bordas, P. ; Borgland, A. ; Borkowski, J. ; Bose, R. ; Botner, O. ; Bottani, A. / Introducing the CTA concept. In: Astroparticle Physics. 2013 ; Vol. 43. pp. 3-18.

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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. {\textcopyright} 2013 Elsevier B.V. All rights reserved.",

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Acharya, BS, Actis, M, Aghajani, T, Agnetta, G, Aguilar, J, Aharonian, F, Ajello, M, Akhperjanian, A, Alcubierre, M, Aleksić, J, Alfaro, R, Aliu, E, Allafort, AJ, Allan, D, Allekotte, I, Amato, E, Anderson, J, Anguner, EO, Antonelli, LA, Antoranz, P, Aravantinos, A, Arlen, T, Armstrong, T, Arnaldi, H, Arrabito, L, Asano, K, Ashton, T, Asorey, HG, Awane, Y, Baba, H, Babic, A, Baby, N, Bahr, J, Bais, A, Baixeras, C, Bajtlik, S, Balbo, M, Balis, D, Balkowski, C, Bamba, A, Bandiera, R, Barber, A, Barbier, C, Barcelo, M, Barnacka, A, Barnstedt, J, De AlmeidaBarres, U, Barrio, JA, Basili, A, Basso, S, Bastieri, D, Bauer, C, Baushev, A, Becerra, J, Becherini, Y, Bechtol, KC, Becker Tjus, J, Beckmann, V, Bednarek, W, Behera, B, Belluso, M, Benbow, W, Berdugo, J, Berger, K, Bernard, F, Bernardino, T, Bernlohr, K, Bhat, N, Bhattacharyya, S, Bigongiari, C, Biland, A, Billotta, S, Bird, T, Birsin, E, Bissaldi, E, Biteau, J, Bitossi, M, Blake, S, Blanch Bigas, O, Blasi, P, Bobkov, A, Boccone, V, Boettcher, M, Bogacz, L, Bogart, J, Bogdan, M, Boisson, C, Boix Gargallo, J, Bolmont, J, Bonanno, G, Bonardi, A, Bonev, T, Bonifacio, P, Bonnoli, G, Bordas, P, Borgland, A, Borkowski, J, Bose, R, Botner, O & Bottani, A 2013, 'Introducing the CTA concept', Astroparticle Physics, vol. 43, pp. 3-18. https://doi.org/10.1016/j.astropartphys.2013.01.007

Introducing the CTA concept. / Acharya, B. S.; Actis, M.; Aghajani, T.; Agnetta, G.; Aguilar, J.; Aharonian, F.; Ajello, M.; Akhperjanian, A.; Alcubierre, M.; Aleksić, J.; Alfaro, R.; Aliu, E.; Allafort, A. J.; Allan, D.; Allekotte, I.; Amato, E.; Anderson, J.; Anguner, E. O.; Antonelli, L. A.; Antoranz, P.; Aravantinos, A.; Arlen, T.; Armstrong, T.; Arnaldi, H.; Arrabito, L.; Asano, K.; Ashton, T.; Asorey, H. G.; Awane, Y.; Baba, H.; Babic, A.; Baby, N.; Bahr, J.; Bais, A.; Baixeras, C.; Bajtlik, S.; Balbo, M.; Balis, D.; Balkowski, C.; Bamba, A.; Bandiera, R.; Barber, A.; Barbier, C.; Barcelo, M.; Barnacka, A.; Barnstedt, J.; De AlmeidaBarres, U.; Barrio, J. A.; Basili, A.; Basso, S.; Bastieri, D.; Bauer, C.; Baushev, A.; Becerra, J.; Becherini, Y.; Bechtol, K. C.; Becker Tjus, J.; Beckmann, V.; Bednarek, W.; Behera, B.; Belluso, M.; Benbow, W.; Berdugo, J.; Berger, K.; Bernard, F.; Bernardino, T.; Bernlohr, K.; Bhat, N.; Bhattacharyya, S.; Bigongiari, C.; Biland, A.; Billotta, S.; Bird, T.; Birsin, E.; Bissaldi, E.; Biteau, J.; Bitossi, M.; Blake, S.; Blanch Bigas, O.; Blasi, P.; Bobkov, A.; Boccone, V.; Boettcher, M.; Bogacz, L.; Bogart, J.; Bogdan, M.; Boisson, C.; Boix Gargallo, J.; Bolmont, J.; Bonanno, G.; Bonardi, A.; Bonev, T.; Bonifacio, P.; Bonnoli, G.; Bordas, P.; Borgland, A.; Borkowski, J.; Bose, R.; Botner, O.; Bottani, A.

In: Astroparticle Physics, Vol. 43, 01.01.2013, p. 3-18.

Research output: Contribution to journal › Article › Research › peer-review

TY - JOUR

T1 - Introducing the CTA concept

AU - Acharya, B. S.

AU - Actis, M.

AU - Aghajani, T.

AU - Agnetta, G.

AU - Aguilar, J.

AU - Aharonian, F.

AU - Ajello, M.

AU - Akhperjanian, A.

AU - Alcubierre, M.

AU - Aleksić, J.

AU - Alfaro, R.

AU - Aliu, E.

AU - Allafort, A. J.

AU - Allan, D.

AU - Allekotte, I.

AU - Amato, E.

AU - Anderson, J.

AU - Anguner, E. O.

AU - Antonelli, L. A.

AU - Antoranz, P.

AU - Aravantinos, A.

AU - Arlen, T.

AU - Armstrong, T.

AU - Arnaldi, H.

AU - Arrabito, L.

AU - Asano, K.

AU - Ashton, T.

AU - Asorey, H. G.

AU - Awane, Y.

AU - Baba, H.

AU - Babic, A.

AU - Baby, N.

AU - Bahr, J.

AU - Bais, A.

AU - Baixeras, C.

AU - Bajtlik, S.

AU - Balbo, M.

AU - Balis, D.

AU - Balkowski, C.

AU - Bamba, A.

AU - Bandiera, R.

AU - Barber, A.

AU - Barbier, C.

AU - Barcelo, M.

AU - Barnacka, A.

AU - Barnstedt, J.

AU - De AlmeidaBarres, U.

AU - Barrio, J. A.

AU - Basili, A.

AU - Basso, S.

AU - Bastieri, D.

AU - Bauer, C.

AU - Baushev, A.

AU - Becerra, J.

AU - Becherini, Y.

AU - Bechtol, K. C.

AU - Becker Tjus, J.

AU - Beckmann, V.

AU - Bednarek, W.

AU - Behera, B.

AU - Belluso, M.

AU - Benbow, W.

AU - Berdugo, J.

AU - Berger, K.

AU - Bernard, F.

AU - Bernardino, T.

AU - Bernlohr, K.

AU - Bhat, N.

AU - Bhattacharyya, S.

AU - Bigongiari, C.

AU - Biland, A.

AU - Billotta, S.

AU - Bird, T.

AU - Birsin, E.

AU - Bissaldi, E.

AU - Biteau, J.

AU - Bitossi, M.

AU - Blake, S.

AU - Blanch Bigas, O.

AU - Blasi, P.

AU - Bobkov, A.

AU - Boccone, V.

AU - Boettcher, M.

AU - Bogacz, L.

AU - Bogart, J.

AU - Bogdan, M.

AU - Boisson, C.

AU - Boix Gargallo, J.

AU - Bolmont, J.

AU - Bonanno, G.

AU - Bonardi, A.

AU - Bonev, T.

AU - Bonifacio, P.

AU - Bonnoli, G.

AU - Bordas, P.

AU - Borgland, A.

AU - Borkowski, J.

AU - Bose, R.

AU - Botner, O.

AU - Bottani, A.

PY - 2013/1/1

Y1 - 2013/1/1

N2 - 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. © 2013 Elsevier B.V. All rights reserved.

AB - 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. © 2013 Elsevier B.V. All rights reserved.

KW - Air showers

KW - Cherenkov Telescopes

KW - TeV gamma-ray astronomy

U2 - 10.1016/j.astropartphys.2013.01.007

DO - 10.1016/j.astropartphys.2013.01.007

M3 - Article

VL - 43

SP - 3

EP - 18

JO - Astroparticle Physics

JF - Astroparticle Physics

SN - 0927-6505

ER -

Introducing the CTA concept

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Keywords

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