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000475430 1001_ $$0V.V.Prosin.1$$aProsin, V.$$b0$$eCorresponding author
000475430 245__ $$aEnergy Spectrum and Mass Composition of Cosmic Rays from the Data of the Astrophysical Complex TAIGA
000475430 260__ $$aNew York, NY$$bAIP$$c2022
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000475430 520__ $$aThe differential energy spectrum of cosmic rays in the energy range of 3 × 10$^{14}$–3 × 10$^{18}$ eV and the corrected dependence of the mean depth of the maximum 〈X$_{max}$〉 of an extensive air shower (EAS) inside the wide energy range of 10$^{15}$–3 × 10$^{17}$ eV have been obtained from the data of the Tunka-133 array for 7 years of operation (2009–2017) and the TAIGA-HiSCORE array for the 2019–2020 season of operation. At the extremely high energy, our results agree with the results of the Pierre Auger Observatory based on direct measurements of the maximum depth by the observation of fluorescent light from EAS. The recalculation from the 〈X$_{max}$〉 to the parameter $\left\langle {\ln A} \right\rangle $, which characterizes the average composition of the primary cosmic rays, is presented.
000475430 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
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000475430 650_7 $$2INSPIRE$$ashowers, atmosphere
000475430 650_7 $$2INSPIRE$$acosmic radiation, energy spectrum
000475430 650_7 $$2INSPIRE$$acosmic radiation, primary
000475430 650_7 $$2INSPIRE$$aradiation, Cherenkov
000475430 650_7 $$2INSPIRE$$acosmic radiation, mass spectrum
000475430 650_7 $$2INSPIRE$$aair
000475430 650_7 $$2INSPIRE$$aAuger
000475430 650_7 $$2INSPIRE$$aobservatory
000475430 650_7 $$2INSPIRE$$aUHE
000475430 650_7 $$2INSPIRE$$afluorescence
000475430 650_7 $$2autogen$$aprimary cosmic rays
000475430 650_7 $$2autogen$$aenergy spectrum
000475430 650_7 $$2autogen$$amass composition
000475430 650_7 $$2autogen$$aextensive air showers
000475430 650_7 $$2autogen$$aCherenkov light
000475430 693__ $$0EXP:(DE-H253)TAIGA-20190101$$5EXP:(DE-H253)TAIGA-20190101$$eTunka Advanced Instrument for cosmic ray physics and Gamma Astronomy$$x0
000475430 7001_ $$0I.I.Astapov.1$$aAstapov, I.$$b1
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000475430 7001_ $$0A.Borodin.1$$aBorodin, A.$$b3
000475430 7001_ $$0P:(DE-H253)PIP1016618$$aBrueckner, Martin$$b4
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000475430 7001_ $$0M.Slunecka.1$$aSlunecka, M.$$b57
000475430 7001_ $$aSokolov, A.$$b58
000475430 7001_ $$aSveshnikova, L.$$b59
000475430 7001_ $$0Y.Suvorkin.1$$aSuvorkin, Y.$$b60
000475430 7001_ $$0V.Tabolenko.1$$aTabolenko, V.$$b61
000475430 7001_ $$0A.B.Tanaev.1$$aTanaev, A.$$b62
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000475430 7001_ $$0L.G.Tkachev.1$$aTkachev, L.$$b65
000475430 7001_ $$0P:(DE-H253)PIP1006705$$aTluczykont, M.$$b66
000475430 7001_ $$aUshakov, N.$$b67
000475430 7001_ $$0A.Vaidyanathan.1$$aVaidyanathan, A.$$b68
000475430 7001_ $$0P.Volchugov.1$$aVolchugov, P.$$b69
000475430 7001_ $$0D.Voronin.4$$aVoronin, D.$$b70
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000475430 7001_ $$0I.V.Yashin.1$$aYashin, I.$$b72
000475430 7001_ $$0A.Zagorodnikov.11$$aZagorodnikov, A.$$b73
000475430 7001_ $$aZhurov, D.$$b74
000475430 7001_ $$0P:(DE-HGF)0$$aThe TAIGA Collaboration$$b75$$eCollaboration author
000475430 773__ $$0PERI:(DE-600)2006377-5$$a10.1134/S1063778821090283$$gVol. 84, no. 9, p. 1653 - 1659$$n9$$p1653 - 1659$$tPhysics of atomic nuclei$$v84$$x1063-7788$$y2022
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