000570292 001__ 570292
000570292 005__ 20250715173533.0
000570292 020__ $$a978-981-12-6976-9
000570292 0247_ $$2doi$$a10.1142/9789811269776_0274
000570292 0247_ $$2INSPIRETeX$$aTluczykont:2023pko
000570292 0247_ $$2inspire$$ainspire:2627643
000570292 0247_ $$2datacite_doi$$a10.3204/PUBDB-2023-00655
000570292 0247_ $$2openalex$$aopenalex:W4317910613
000570292 037__ $$aPUBDB-2023-00655
000570292 041__ $$aEnglish
000570292 1001_ $$0P:(DE-H253)PIP1006705$$aTluczykont, M.$$b0
000570292 1112_ $$a16th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories$$cOnline$$d2021-07-05 - 2021-07-09$$gMG16$$wItaly
000570292 245__ $$aThe TAIGA experiment
000570292 260__ $$bWorld Scientific Publishing$$c2023
000570292 29510 $$aThe Sixteenth Marcel Grossmann Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories (In 4 Volumes)
000570292 300__ $$a3324-3342
000570292 3367_ $$2ORCID$$aCONFERENCE_PAPER
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000570292 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1676372465_22602
000570292 3367_ $$0PUB:(DE-HGF)7$$2PUB:(DE-HGF)$$aContribution to a book$$mcontb
000570292 4900_ $$2Author
000570292 520__ $$aThe Tunka Advanced Instrument for Gamma-ray and cosmic ray Astrophysics (TAIGA) is a hybrid experiment for the measurement of Extensive Air Showers (EAS) with good spectral resolution in the TeV to PeV energy range. In this domain, the long-sought Pevatrons can be detected. Currently the hybrid TAIGA detector combines two wide angle shower front Cherenkov light sampling timing arrays (HiSCORE and Tunka-133), two 4m class, 10° aperture Imaging Air Cherenkov Telescopes (IACTs) and 240 m2 surface and underground charged particle detector stations. Our goal is to introduce a new hybrid reconstruction technique, combining the good angular and shower core resolution of HiSCORE with the gamma-hadron separation power of imaging telescopes. This approach allows to maximize the effective area and simultaneously to reach a good gamma-hadron separation at low energies (few TeV). At higher energies, muon detectors are planned to enhance gamma-hadron separation. During the commissioning phase of the first and second IACT, several sources were observed. First detections of known sources with the first telescope show the functionality of the TAIGA IACTs. Here, the status of the TAIGA experiment will be presented, along with first results from the current configuration.
000570292 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000570292 588__ $$aDataset connected to CrossRef Conference, INSPIRE
000570292 650_7 $$2INSPIRE$$aradiation, Cherenkov
000570292 650_7 $$2INSPIRE$$abeam, width
000570292 650_7 $$2INSPIRE$$adetector, imaging
000570292 650_7 $$2INSPIRE$$acharged particle, detector
000570292 650_7 $$2INSPIRE$$aenergy, high
000570292 650_7 $$2INSPIRE$$ashowers, atmosphere
000570292 650_7 $$2INSPIRE$$amuon, detector
000570292 650_7 $$2INSPIRE$$aenergy, low
000570292 650_7 $$2INSPIRE$$ahybrid
000570292 650_7 $$2INSPIRE$$aair
000570292 650_7 $$2INSPIRE$$agamma ray
000570292 650_7 $$2INSPIRE$$aresolution
000570292 650_7 $$2INSPIRE$$aTeV
000570292 650_7 $$2INSPIRE$$aspectral
000570292 650_7 $$2INSPIRE$$acosmic radiation
000570292 650_7 $$2INSPIRE$$awide-angle
000570292 650_7 $$2INSPIRE$$asurface
000570292 650_7 $$2INSPIRE$$aCherenkov counter
000570292 650_7 $$2autogen$$aGamma-rays: experiments
000570292 650_7 $$2autogen$$aObservations: Crab Nebula
000570292 693__ $$0EXP:(DE-H253)TAIGA-20190101$$5EXP:(DE-H253)TAIGA-20190101$$eTunka Advanced Instrument for cosmic ray physics and Gamma Astronomy$$x0
000570292 7001_ $$0I.I.Astapov.1$$aAstapov, I. I.$$b1
000570292 7001_ $$0A.K.Awad.1$$aAwad, A. K.$$b2
000570292 7001_ $$0P.A.Bezyazeekov.4$$aBezyazeekov, P. A.$$b3
000570292 7001_ $$aBlank, M.$$b4
000570292 7001_ $$0E.A.Bonvech.1$$aBonvech, E. A.$$b5
000570292 7001_ $$0A.N.Borodin.1$$aBorodin, A. N.$$b6
000570292 7001_ $$0A.V.Bulan.1$$aBulan, A. V.$$b7
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000570292 7001_ $$0A.Chiavassa.1$$aChiavassa, A.$$b10
000570292 7001_ $$0D.V.Chernov.8$$aChernov, D. V.$$b11
000570292 7001_ $$0A.Dyachok.1$$aDyachok, A. N.$$b12
000570292 7001_ $$0A.R.Gafarov.1$$aGafarov, A. R.$$b13
000570292 7001_ $$aGarmash, A. Yu.$$b14
000570292 7001_ $$0V.M.Grebenyuk.1$$aGrebenyuk, V. M.$$b15
000570292 7001_ $$0O.A.Gress.1$$aGress, O. A.$$b16
000570292 7001_ $$0E.Gress.1$$aGress, E.$$b17
000570292 7001_ $$0T.I.Gress.13$$aGress, T. I.$$b18
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000570292 7001_ $$aIvanova, A. L.$$b22
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000570292 7001_ $$aKorosteleva, E. E.$$b28
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000570292 7001_ $$0E.A.Kravchenko.2$$aKravchenko, E. A.$$b30
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000570292 7001_ $$aKuzmichev, L. A.$$b32
000570292 7001_ $$0A.A.Lagutin.1$$aLagutin, A. A.$$b33
000570292 7001_ $$0M.V.Lavrova.1$$aLavrova, M.$$b34
000570292 7001_ $$0Y.E.Lemeshev.1$$aLemeshev, E.$$b35
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000570292 7001_ $$0A.D.Lukanov.1$$aLukanov, A. D.$$b38
000570292 7001_ $$0D.Lukyantsev.1$$aLukyantsev, D. S.$$b39
000570292 7001_ $$0R.R.Mirgazov.9$$aMirgazov, R. R.$$b40
000570292 7001_ $$0R.Mirzoyan.1$$aMirzoyan, R.$$b41
000570292 7001_ $$0R.D.Monkhoev.1$$aMonkhoev, R. D.$$b42
000570292 7001_ $$aOsipova, E. A.$$b43
000570292 7001_ $$0A.L.Pakhorukov.1$$aPakhorukov, A. L.$$b44
000570292 7001_ $$aPan, A.$$b45
000570292 7001_ $$aPankov, L. V.$$b46
000570292 7001_ $$0A.D.Panov.1$$aPanov, A. D.$$b47
000570292 7001_ $$aPetrukhin, A. A.$$b48
000570292 7001_ $$0D.A.Podgrudkov.1$$aPodgrudkov, D. A.$$b49
000570292 7001_ $$0V.Poleschuk.1$$aPoleschuk, V. A.$$b50
000570292 7001_ $$aPopova, E. G.$$b51
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000570292 7001_ $$0Y.A.Semeney.1$$aSemeney, Yu. A.$$b64
000570292 7001_ $$0A.A.Silaev.2$$aSilaev, A. A.$$b65
000570292 7001_ $$0A.A.Silaev.2$$aSilaev, A. A.$$b66
000570292 7001_ $$0A.Y.Sidorenkov.1$$aSidorenkov, A. Yu.$$b67
000570292 7001_ $$0A.V.Skurikhin.1$$aSkurikhin, A. V.$$b68
000570292 7001_ $$aSokolov, A. V.$$b69
000570292 7001_ $$0Y.Suvorkin.1$$aSuvorkin, Y.$$b70
000570292 7001_ $$aSveshnikova, L. G.$$b71
000570292 7001_ $$0V.A.Tabolenko.2$$aTabolenko, V. A.$$b72
000570292 7001_ $$0A.B.Tanaev.1$$aTanaev, A. B.$$b73
000570292 7001_ $$0B.Tarashansky.2$$aTarashansky, B. A.$$b74
000570292 7001_ $$0M.Ternovoy.1$$aTernovoy, M.$$b75
000570292 7001_ $$0L.G.Tkachev.1$$aTkachev, L. G.$$b76
000570292 7001_ $$aUshakov, N.$$b77
000570292 7001_ $$0A.Vaidyanathan.1$$aVaidyanathan, A.$$b78
000570292 7001_ $$0P.A.Volchugov.1$$aVolchugov, P. A.$$b79
000570292 7001_ $$aVolkov, N. V.$$b80
000570292 7001_ $$0D.Voronin.14$$aVoronin, D.$$b81
000570292 7001_ $$0P:(DE-H253)PIP1003748$$aWischnewski, R.$$b82
000570292 7001_ $$0I.V.Yashin.1$$aYashin, I. I.$$b83
000570292 7001_ $$0A.V.Zagorodnikov.1$$aZagorodnikov, A. V.$$b84
000570292 7001_ $$aZhurov, D. P.$$b85
000570292 7001_ $$0P:(DE-HGF)0$$aTAIGA Collaboration$$b86$$eCollaboration author
000570292 773__ $$a10.1142/9789811269776_0274
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