Research output: Contribution to journal › Article › peer-review
Detection of TeV Emission from the Crab Nebula Using the First Two IACTs in TAIGA in Stereo Mode of Observation. / the TAIGA Collaboration ; Вайдянатан, Арун .
In: Physics of Atomic Nuclei, Vol. 86, No. 4, 08.2023, p. 483-488.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Detection of TeV Emission from the Crab Nebula Using the First Two IACTs in TAIGA in Stereo Mode of Observation
AU - the TAIGA Collaboration
AU - Volchugov, P. A.
AU - Astapov, I. I.
AU - Bezyazeekov, P. A.
AU - Bonvech, E. A.
AU - Borodin, A.
AU - Budnev, N.
AU - Bulan, A. V.
AU - Chiavassa, A.
AU - Chernov, D. V.
AU - Dyachok, A.
AU - Gafarov, A.
AU - Garmash, A.
AU - Grebenyuk, V.
AU - Gress, O.
AU - Gress, E.
AU - Gress, T.
AU - Grinyuk, A.
AU - Grishin, O.
AU - Ivanova, A. D.
AU - Ivanova, A. L.
AU - Ilushin, M.
AU - Kalmykov, N.
AU - Kindin, V.
AU - Kiryuhin, S.
AU - Kokoulin, R.
AU - Kolosov, N.
AU - Kompaniets, K.
AU - Korosteleva, E.
AU - Kozhin, V.
AU - Kravchenko, E.
AU - Kryukov, A.
AU - Kuzmichev, L.
AU - Lagutin, A.
AU - Lavrova, M.
AU - Lemeshev, Y. E.
AU - Lubsandorzhiev, B.
AU - Lubsandorzhiev, N.
AU - Malakhov, S. D.
AU - Mirgazov, R.
AU - Monkhoev, R.
AU - Osipova, E.
AU - Okuneva, E.
AU - Pakhorukov, A.
AU - Pan, A.
AU - Pankov, L.
AU - Panov, A. D.
AU - Petrukhin, A.
AU - Podgrudkov, D. A.
AU - Rubtsov, G.
AU - Sokolov, A.
AU - Вайдянатан, Арун
N1 - The work was performed at the UNU ‘‘Astrophysical Complex of MSU-ISU’’ (agreement EB-075-15-2021-675). The work is supported the Russian Federation Ministry of Science and High Education (projects FZZE-2020-0024 and FZZE-2023-0004) and by Russian Foundation for Basic Research, grant 23-72-00019 (Sections 3–6, 23-72-00016). Публикация для корректировки.
PY - 2023/8
Y1 - 2023/8
N2 - This paper presents the results of an analysis of observations of the Crab Nebula gamma-ray source with the first two atmospheric Cherenkov telescopes of the TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) astrophysical complex in the stereo mode of observations. The article analyzed observational data from 2020 to 2021. Over 36 hours of observations, a signal was obtained at a statistical significance level of 5σ and a spectrum of gamma rays was plotted in the energy range from 2 to 70 TeV. The paper describes a technique for gamma–hadron separation and reconstruction of detected gamma-rays energy.
AB - This paper presents the results of an analysis of observations of the Crab Nebula gamma-ray source with the first two atmospheric Cherenkov telescopes of the TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) astrophysical complex in the stereo mode of observations. The article analyzed observational data from 2020 to 2021. Over 36 hours of observations, a signal was obtained at a statistical significance level of 5σ and a spectrum of gamma rays was plotted in the energy range from 2 to 70 TeV. The paper describes a technique for gamma–hadron separation and reconstruction of detected gamma-rays energy.
UR - https://www.scopus.com/record/display.uri?eid=2-s2.0-85169679831&origin=inward&txGid=98b48de71d9bfc40776477e4e789cca1
UR - https://www.mendeley.com/catalogue/c754fcb9-fc80-3a36-9a0f-f84739e85e48/
U2 - 10.1134/S1063778823040385
DO - 10.1134/S1063778823040385
M3 - Article
VL - 86
SP - 483
EP - 488
JO - Physics of Atomic Nuclei
JF - Physics of Atomic Nuclei
SN - 1063-7788
IS - 4
ER -
ID: 59563672