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001     570292
005     20250715173533.0
020 _ _ |a 978-981-12-6976-9
024 7 _ |a 10.1142/9789811269776_0274
|2 doi
024 7 _ |a Tluczykont:2023pko
|2 INSPIRETeX
024 7 _ |a inspire:2627643
|2 inspire
024 7 _ |a 10.3204/PUBDB-2023-00655
|2 datacite_doi
024 7 _ |2 openalex
|a openalex:W4317910613
037 _ _ |a PUBDB-2023-00655
041 _ _ |a English
100 1 _ |a Tluczykont, M.
|0 P:(DE-H253)PIP1006705
|b 0
111 2 _ |a 16th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories
|g MG16
|c Online
|d 2021-07-05 - 2021-07-09
|w Italy
245 _ _ |a The TAIGA experiment
260 _ _ |c 2023
|b World Scientific Publishing
295 1 0 |a The Sixteenth Marcel Grossmann Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories (In 4 Volumes)
300 _ _ |a 3324-3342
336 7 _ |a CONFERENCE_PAPER
|2 ORCID
336 7 _ |a Conference Paper
|0 33
|2 EndNote
336 7 _ |a INPROCEEDINGS
|2 BibTeX
336 7 _ |a conferenceObject
|2 DRIVER
336 7 _ |a Output Types/Conference Paper
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336 7 _ |a Contribution to a conference proceedings
|b contrib
|m contrib
|0 PUB:(DE-HGF)8
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336 7 _ |a Contribution to a book
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|2 PUB:(DE-HGF)
|m contb
490 0 _ |2 Author
520 _ _ |a The 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.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
|0 G:(DE-HGF)POF4-613
|c POF4-613
|f POF IV
|x 0
588 _ _ |a Dataset connected to CrossRef Conference, INSPIRE
650 _ 7 |a radiation, Cherenkov
|2 INSPIRE
650 _ 7 |a beam, width
|2 INSPIRE
650 _ 7 |a detector, imaging
|2 INSPIRE
650 _ 7 |a charged particle, detector
|2 INSPIRE
650 _ 7 |a energy, high
|2 INSPIRE
650 _ 7 |a showers, atmosphere
|2 INSPIRE
650 _ 7 |a muon, detector
|2 INSPIRE
650 _ 7 |a energy, low
|2 INSPIRE
650 _ 7 |a hybrid
|2 INSPIRE
650 _ 7 |a air
|2 INSPIRE
650 _ 7 |a gamma ray
|2 INSPIRE
650 _ 7 |a resolution
|2 INSPIRE
650 _ 7 |a TeV
|2 INSPIRE
650 _ 7 |a spectral
|2 INSPIRE
650 _ 7 |a cosmic radiation
|2 INSPIRE
650 _ 7 |a wide-angle
|2 INSPIRE
650 _ 7 |a surface
|2 INSPIRE
650 _ 7 |a Cherenkov counter
|2 INSPIRE
650 _ 7 |a Gamma-rays: experiments
|2 autogen
650 _ 7 |a Observations: Crab Nebula
|2 autogen
693 _ _ |0 EXP:(DE-H253)TAIGA-20190101
|5 EXP:(DE-H253)TAIGA-20190101
|e Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy
|x 0
700 1 _ |a Astapov, I. I.
|0 I.I.Astapov.1
|b 1
700 1 _ |a Awad, A. K.
|0 A.K.Awad.1
|b 2
700 1 _ |a Bezyazeekov, P. A.
|0 P.A.Bezyazeekov.4
|b 3
700 1 _ |a Blank, M.
|b 4
700 1 _ |a Bonvech, E. A.
|0 E.A.Bonvech.1
|b 5
700 1 _ |a Borodin, A. N.
|0 A.N.Borodin.1
|b 6
700 1 _ |a Bulan, A. V.
|0 A.V.Bulan.1
|b 7
700 1 _ |a Brückner, M.
|0 P:(DE-H253)PIP1016618
|b 8
700 1 _ |a Budnev, N. M.
|0 N.M.Budnev.11
|b 9
700 1 _ |a Chiavassa, A.
|0 A.Chiavassa.1
|b 10
700 1 _ |a Chernov, D. V.
|0 D.V.Chernov.8
|b 11
700 1 _ |a Dyachok, A. N.
|0 A.Dyachok.1
|b 12
700 1 _ |a Gafarov, A. R.
|0 A.R.Gafarov.1
|b 13
700 1 _ |a Garmash, A. Yu.
|b 14
700 1 _ |a Grebenyuk, V. M.
|0 V.M.Grebenyuk.1
|b 15
700 1 _ |a Gress, O. A.
|0 O.A.Gress.1
|b 16
700 1 _ |a Gress, E.
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|b 17
700 1 _ |a Gress, T. I.
|0 T.I.Gress.13
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700 1 _ |a Grishin, O. G.
|0 O.G.Grishin.3
|b 19
700 1 _ |a Grinyuk, A. A.
|0 A.Grinyuk.1
|b 20
700 1 _ |a Horns, D.
|0 P:(DE-H253)PIP1006257
|b 21
700 1 _ |a Ivanova, A. L.
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700 1 _ |a Kalmykov, N. N.
|0 N.N.Kalmykov.8
|b 23
700 1 _ |a Kindin, V. V.
|0 V.V.Kindin.1
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700 1 _ |a Kiryuhin, S. N.
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|b 25
700 1 _ |a Kokoulin, R. P.
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|b 26
700 1 _ |a Kompaniets, K. G.
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|b 27
700 1 _ |a Korosteleva, E. E.
|b 28
700 1 _ |a Kozhin, V. A.
|0 V.A.Kozhin.13
|b 29
700 1 _ |a Kravchenko, E. A.
|0 E.A.Kravchenko.2
|b 30
700 1 _ |a Kryukov, A. P.
|0 A.Kryukov.1
|b 31
700 1 _ |a Kuzmichev, L. A.
|b 32
700 1 _ |a Lagutin, A. A.
|0 A.A.Lagutin.1
|b 33
700 1 _ |a Lavrova, M.
|0 M.V.Lavrova.1
|b 34
700 1 _ |a Lemeshev, E.
|0 Y.E.Lemeshev.1
|b 35
700 1 _ |a Lubsandorzhiev, B. K.
|0 B.K.Lubsandorzhiev.1
|b 36
700 1 _ |a Lubsandorzhiev, N. B.
|0 N.B.Lubsandorzhiev.1
|b 37
700 1 _ |a Lukanov, A. D.
|0 A.D.Lukanov.1
|b 38
700 1 _ |a Lukyantsev, D. S.
|0 D.Lukyantsev.1
|b 39
700 1 _ |a Mirgazov, R. R.
|0 R.R.Mirgazov.9
|b 40
700 1 _ |a Mirzoyan, R.
|0 R.Mirzoyan.1
|b 41
700 1 _ |a Monkhoev, R. D.
|0 R.D.Monkhoev.1
|b 42
700 1 _ |a Osipova, E. A.
|b 43
700 1 _ |a Pakhorukov, A. L.
|0 A.L.Pakhorukov.1
|b 44
700 1 _ |a Pan, A.
|b 45
700 1 _ |a Pankov, L. V.
|b 46
700 1 _ |a Panov, A. D.
|0 A.D.Panov.1
|b 47
700 1 _ |a Petrukhin, A. A.
|b 48
700 1 _ |a Podgrudkov, D. A.
|0 D.A.Podgrudkov.1
|b 49
700 1 _ |a Poleschuk, V. A.
|0 V.Poleschuk.1
|b 50
700 1 _ |a Popova, E. G.
|b 51
700 1 _ |a Porelli, A.
|0 P:(DE-H253)PIP1017590
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700 1 _ |a Postnikov, E. B.
|0 E.Postnikov.1
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700 1 _ |a Prosin, V. V.
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|b 54
700 1 _ |a Ptuskin, V. S.
|0 V.S.Ptuskin.1
|b 55
700 1 _ |a Pushnin, A. A.
|0 A.A.Pushnin.1
|b 56
700 1 _ |a Raikin, R. I.
|0 R.Raikin.1
|b 57
700 1 _ |a Razumov, A. Y.
|0 I.A.Razumov.1
|b 58
700 1 _ |a Rubtsov, G. I.
|0 G.I.Rubtsov.1
|b 59
700 1 _ |a Ryabov, E. V.
|0 E.V.Ryabov.1
|b 60
700 1 _ |a Sagan, Y. I.
|0 Y.I.Sagan.1
|b 61
700 1 _ |a Samoliga, V. S.
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|b 62
700 1 _ |a Satyshev, I.
|0 I.Satyshev.1
|b 63
700 1 _ |a Semeney, Yu. A.
|0 Y.A.Semeney.1
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700 1 _ |a Silaev, A. A.
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|b 65
700 1 _ |a Silaev, A. A.
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700 1 _ |a Sidorenkov, A. Yu.
|0 A.Y.Sidorenkov.1
|b 67
700 1 _ |a Skurikhin, A. V.
|0 A.V.Skurikhin.1
|b 68
700 1 _ |a Sokolov, A. V.
|b 69
700 1 _ |a Suvorkin, Y.
|0 Y.Suvorkin.1
|b 70
700 1 _ |a Sveshnikova, L. G.
|b 71
700 1 _ |a Tabolenko, V. A.
|0 V.A.Tabolenko.2
|b 72
700 1 _ |a Tanaev, A. B.
|0 A.B.Tanaev.1
|b 73
700 1 _ |a Tarashansky, B. A.
|0 B.Tarashansky.2
|b 74
700 1 _ |a Ternovoy, M.
|0 M.Ternovoy.1
|b 75
700 1 _ |a Tkachev, L. G.
|0 L.G.Tkachev.1
|b 76
700 1 _ |a Ushakov, N.
|b 77
700 1 _ |a Vaidyanathan, A.
|0 A.Vaidyanathan.1
|b 78
700 1 _ |a Volchugov, P. A.
|0 P.A.Volchugov.1
|b 79
700 1 _ |a Volkov, N. V.
|b 80
700 1 _ |a Voronin, D.
|0 D.Voronin.14
|b 81
700 1 _ |a Wischnewski, R.
|0 P:(DE-H253)PIP1003748
|b 82
700 1 _ |a Yashin, I. I.
|0 I.V.Yashin.1
|b 83
700 1 _ |a Zagorodnikov, A. V.
|0 A.V.Zagorodnikov.1
|b 84
700 1 _ |a Zhurov, D. P.
|b 85
700 1 _ |a TAIGA Collaboration
|0 P:(DE-HGF)0
|b 86
|e Collaboration author
773 _ _ |a 10.1142/9789811269776_0274
856 4 _ |y OpenAccess
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910 1 _ |a External Institute
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910 1 _ |a Deutsches Elektronen-Synchrotron
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910 1 _ |a Deutsches Elektronen-Synchrotron
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913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-613
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
|4 G:(DE-HGF)POF
|v Matter and Radiation from the Universe
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914 1 _ |y 2023
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915 _ _ |a Creative Commons Attribution CC BY 4.0
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920 1 _ |0 I:(DE-H253)Z_GA-20210408
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|l Gammaastronomie
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980 _ _ |a contrib
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a contb
980 _ _ |a I:(DE-H253)Z_GA-20210408
980 1 _ |a FullTexts

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