Abstract
The Earth is continuously bombarded by cosmic rays and gamma-rays extending over an immense range of energies. Discovered in 1912 by Victor Hess, the cosmic radiation has been studied from balloons, from space, from the ground, and from underground. The resulting fields of cosmic-ray astrophysics (focused on the charged particles), gamma-ray astrophysics, and neutrino astrophysics have diverged somewhat. But for the air showers in the GeV and TeV energy ranges, the ground-based detector techniques have considerable overlaps.
Very high-energy (VHE) gamma-ray astronomy is the observational study measuring the directions, flux, energy spectra, and time variability of the sources of these gamma-rays. These measurements constrain the theoretical models of the sources and their interactions between the sources and detection at Earth. With the low flux of gamma-rays, and the background of charged particle cosmic rays, the distinguishing characteristic of gamma-ray air shower detectors is large size and significant photon to charge particle discrimination.
Air shower telescopes for gamma-ray astronomy consist of an array of detectors capable of measuring the passage of particles through the array elements. To maximize signal at energies of a TeV or so, the array needs to be built at high altitude as the maximum number of shower particles is high in the atmosphere. These detectors have included sparse arrays of shower counters, dense arrays of scintillators or resistive plate counters (RPC), buried muon detectors in concert with surface detectors, or many-interaction-deep water Cherenkov detectors (WCD).
In general, these detectors are sensitive over a large field of view, and the whole of the sky is a typical sensitivity and perhaps two-thirds of the sky selected for clean analysis, but with only moderate resolution in energy, typically due to shower-to-shower fluctuations and the intrinsic sampling of the detector. These telescopes, though, operate continuously, despite weather, moonlight, day or night, and without needing to be pointed to a specific target for essentially a 100% duty cycle. In this chapter, we will examine the performance and characteristics of such detectors. These are contrasted with the Imaging Air Cherenkov Telescopes which also operate in this energy range, and both current and future proposed experiments are described.
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References
M.G. Aartsen, M. Ackermann, J. Adams, J.A. Aguilar et al. ICETOP Collaboration, Cosmic ray spectrum and composition from PeV to EeV using 3 years of data from IceTop and IceCube. Phys. Rev. D 100, 082002 (2019)
H. Abdalla et al. (2021) arXiv:2107.01425
A.U. Abeysekara et al. (HAWC), Astropart. Phys. 35, 641–650 (2012). (Preprint 1108.6034)
A.U. Abeysekara et al. (HAWC), Astropart. Phys. 50–52, 26–32 (2013). (Preprint 1306.5800)
A.U. Abeysekara et al. (HAWC), Astrophys. J. 841, 100 (2017). (Preprint 1703.06968)
A.U. Abeysekara et al., NIM A888, 138 (2018a)
A.U. Abeysekara et al. (HAWC Collaboration), Phys. Rev. D 97, 102005 (2018b)
A.U. Abeysekara et al. (HAWC Collaboration), Phys. Rev. Lett. 124, 021102 (2020)
M. Aglietta, G. Di Sciascio et al. (EAS-TOP Collaboration), Astropart. Phys. 3, 1 (1995)
F. Aharonian et al. (HEGRA Collaboration), Astroph. J. 614, 897 (2004)
G. Aielli et al. (ARGO-YBJ Collaboration), Nucl. Instrum. Methods Phys. Res. Sect. A 562, 92 (2006)
G. Aielli et al. (ARGO-YBJ Collaboration), Nucl. Instrum. Methods Phys. Res. Sect. A 608, 246 (2009)
A. Albert et al., (2019). arXiv:1902.08429; M. Mostafa et al., PoS ICRC2017, 851 (2018). https://www.swgo.org/
D.E. Alexandreas et al., Nucl. Instrum. Methods A 311, 350 (1992)
M. Amenomori, X.J. Bi, D. Chen, S.W. Cui, L.K. Ding et al., Tibet ASγ Collaboration, Cosmic-ray energy spectrum around the knee obtained by the Tibet experiment and future prospects. Adv. Space Res. 47, 629 (2011)
M. Amenomori et al., Tibet ASγ collaboration. ApJ 813, 98 (2015)
M. Amenomori et al. (Tibet ASγ Collaboration), Phys. Rev. Lett. 123, 051101 (2019); M. Amenomori et al. (Tibet ASg Collaboration), Phys. Rev. Lett. 126, 141101 (2021)
T. Antoni, W.D. Apel, A.F. Badea, K. Bekk, A. Bercuci et al., KASCADE Collaboration, KASCADE measurements of energy spectra for elemental groups of cosmic rays: results and open problems. Astropart. Phys. 24, 1 (2005)
W.D. Apel, J.C. Arteaga-Velázquez, K. Bekk, M. Bertainaet et al., KASCADE-Grande Collaboration, The spectrum of high-energy cosmic rays measured with KASCADE-Grande. Astropart. Phys. 36, 183 (2012)
T. Asaba et al. (ALPACA Collaboration), PoS ICRC2017, 827 (2018). https://alpaca-experiment.org/
P. Assis et al., Astropart. Phys. 99, 34 (2018)
R. Atkins et al., Nucl. Instrum. Methods Phys. Res. 449 478 (2000)
H.A. Ayala Solares et al., Astropart.Phys. 114, 68 (2020). https://www.amon.psu.edu/
C. Bacci et al. (ARGO-YBJ Collaboration), Nucl. Instrum. Methods Phys. Res. Sect. A 443, 342 (2000)
C. Bacci et al., Astropart. Phys. 17, 151 (2002)
B. Bartoli, P. Bernardini, X.J. Bi, C. Bleve, I. Bolognino et al., ARGO-YBJ Collaboration, Observation of the cosmic ray moon shadowing effect with the ARGO-YBJ experiment. Phys. Rev. D84, 022003 (2011)
B. Bartoli et al. (ARGO-YBJ Collaboration), Astropart. Phys. 67, 47 (2015a)
B. Bartoli et al. (ARGO-YBJ), Astrophys. J. 798, 119 (2015b). (Preprint 1502.05665)
Y. Becherini et al., PoS ICRC2017, 782 (2018)
A. Borione et al., Nucl. Instrum. Methods A 346, 329 (1994)
A. Borione et al. (CASA-MIA Collaboration), Phys. Rev. D 55, 1714 (1997)
Z. Cao, LHAASO Collaboration, Ultrahigh-energy photons up to 1.4 petaelectronvolts from 12 γ-ray Galactic sources. Nature 594, 33–36 (2021)
J.W. Cronin, Nuovo Cimento 19C, 847 (1996)
B. D’Ettorre Piazzoli, G. Di Sciascio, Astropart. Phys. 2, 199 (1994): erratum 327
G. Di Sciascio, Int. J. Mod. Phys. D23, 1430019 (2014); [Erratum: Int. J. Mod. Phys. D24(02), 1592001 (2014)]
G. Di Sciascio (LHAASO), Nucl. Part. Phys. Proc. 279–281, 166–173 (2016). (Preprint 1602.07600)
G. Di Sciascio, J. Phys. Conf. Ser. 1263, 012003 (2019)
G. Di Sciascio et al. (STACEX Collaboration), (2019) arXiv:1907.06686
G. Di Sciascio, B. D’Ettorre Piazzoli, M. Iacovacci, Astropart. Phys. 6, 313 (1997)
G. Di Sciascio et al., Proceedings of the 28th International Cosmic Ray Conference (ICRC 03), Tsukuba, Japan vol. 5 (Universal Academy Press, Inc., Tokyo, 2003), p. 3015
G. Di Sciascio et al. (ARGO-YBJ Collaboration), in International Cosmic Ray Conference (ICRC 05), Pune, India, ed. by B.S. Acharya, S. Gupta, S. Tonwar, vol. 6 (Tata Institute of Fundamental Research, Mumbai, 2005), p. 33
G. Di Sciascio, S. Miozzi, P. Montini, G. Piano, R. Santonico, M. Tavani, PoS ICRC2017, 781 (2018)
R. Engel, D. Heck, T. Pierog. Annu. Rev. Nucl. Part. Sci. 61, 467 (2011)
M.A.K. Glasmacher, M.A. Catanese, M.C. Chantell et al., CASA-MIA Collaboration, The cosmic ray composition between 1014 and 1016 eV. Astropart. Phys. 12, 1 (1999)
K. Greisen, Progr. Cosmic Rays 3, 1 (1956)
W. Heitler, The Quantum Theory of Radiation (Clarendon Press/Oxford, London, 1944)
J.R. Horandel, Astrop. Phys. 19, 193 (2003)
A. Karle et al., Astropart. Phys. 3, 321 (1995)
A. Krys et al., J. Phys. G: Nucl. Part. Phys. 17, 1261 (1991)
S. Kunwar et al., Eur. Phys. J. C in submission (2021)
J. Matthews, Astropart. Phys. 22, 387 (2005)
R. Maze, A. Zawadzki, Nuovo Cimento 17, 625 (1960)
NOAO, NASA, and USAF, US Standard Atmosphere 1976, US Government Printing Office (1976)
V.V. Prosin, S.F. Berezhnev, N.M. Budnev et al., TUNKA Collaboration, Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype. EPJ Web Conf. 121, 03004 (2016)
R.J. Protheroe, R.W. Clay, Proc. ASA 5, 586 (1984)
H. Schoorlemmer et al., Eur. Phys. J. C 79, 427 (2019)
G. Sinnis, WSPC Handb. Astron. Instrum. 7, 137 (2021)
S. Westerhoff (HAWC Collaboration), Adv. Space Res. 53, 1492 (2014)
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DuVernois, M.A., Sciascio, G.D. (2023). Detecting Gamma-Rays with Moderate Resolution and Large Field of View: Particle Detector Arrays and Water Cherenkov Technique. In: Bambi, C., Santangelo, A. (eds) Handbook of X-ray and Gamma-ray Astrophysics. Springer, Singapore. https://doi.org/10.1007/978-981-16-4544-0_64-1
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