Gamma-hadron separation approach to point-like source observations in the TAIGA-IACT experiment in stereo observation mode

Standard

Gamma-hadron separation approach to point-like source observations in the TAIGA-IACT experiment in stereo observation mode. / the TAIGA Collaboration ; Вайдянатан, Арун .

In: Proceedings of Science, Vol. 444, 686, 27.09.2024.

Research output: Contribution to journal › Conference article › peer-review

BibTeX

@article{5417d3f6e3694322822dc3b7b8eafd8f,

title = "Gamma-hadron separation approach to point-like source observations in the TAIGA-IACT experiment in stereo observation mode",

abstract = "This paper is devoted to the analysis of simulation results of TAIGA-IACT in stereo mode of observations and describes the technique of gamma-ray detection with energies higher than several TeV. TAIGA-IACT is part of the TAIGA astrophysics complex. Installation currently consists of three operating telescopes located 300-500 m apart. Two additional telescopes will begin operation in the next two years. We describe a new gamma-hadron separation technique for point-like source observations.",

author = "{the TAIGA Collaboration} and Togoo Ravdandorj and P. Volchugov and I. Astapov and Bezyazeekov, {P. A.} and Blinov, {A. E.} and Bonvech, {E. A.} and A. Borodin and Budnev, {N. M.} and A. Bulan and A. Chiavassa and Chernov, {D. V.} and Dyachok, {A. N.} and Gafarov, {A. R.} and A. Garmash and V. Grebenyuk and O. Gress and E. Gress and Gress, {T. I.} and A. Grinyuk and O. Grishin and A. Ivanova and M. Ilushin and N. Kalmykov and V. Kindin and S. Kiryuhin and R. Kokoulin and N. Kolosov and K. Kompaniets and E. Korosteleva and Kozhin, {V. A.} and E. Kravchenko and A. Kryukov and L. Kuzmichev and A. Lagutin and M. Lavrova and Lemeshev, {Y. E.} and B. Lubsandorzhiev and N. Lubsandorzhiev and S. Malakhov and Mirgazov, {R. R.} and R. Monkhoev and E. Osipova and E. Okuneva and A. Pakhorukov and A. Pan and L. Pankov and A. Panov and G. Rubtsov and V. Samoliga and A. Sokolov and Арун Вайдянатан",

note = "The work was performed at the UNU “Astrophysical Complex of MSU-ISU” (agreement 13.UNU.21.0007). The work is supported by the Russian Science Foundation (grant 23-72-00019 (sections 3 – 5)). The authors would like to thank Irkutsk Supercomputer Center of SB RAS for providing the access to HPC-cluster «Akademik V.M. Matrosov» (Irkutsk Supercomputer Center of SB RAS, Irkutsk: ISDCT SB RAS; http://hpc.icc.ru, accessed 13.07.2023). Публикация для корректировки.; 38th International Cosmic Ray Conference, ICRC 2023 ; Conference date: 26-07-2023 Through 03-08-2023",

year = "2024",

month = sep,

day = "27",

doi = "10.22323/1.444.0686",

language = "English",

volume = "444",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

RIS

TY - JOUR

T1 - Gamma-hadron separation approach to point-like source observations in the TAIGA-IACT experiment in stereo observation mode

AU - the TAIGA Collaboration

AU - Ravdandorj, Togoo

AU - Volchugov, P.

AU - Astapov, I.

AU - Bezyazeekov, P. A.

AU - Blinov, A. E.

AU - Bonvech, E. A.

AU - Borodin, A.

AU - Budnev, N. M.

AU - Bulan, A.

AU - Chiavassa, A.

AU - Chernov, D. V.

AU - Dyachok, A. N.

AU - Gafarov, A. R.

AU - Garmash, A.

AU - Grebenyuk, V.

AU - Gress, O.

AU - Gress, E.

AU - Gress, T. I.

AU - Grinyuk, A.

AU - Grishin, O.

AU - Ivanova, A.

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. A.

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.

AU - Mirgazov, R. R.

AU - Monkhoev, R.

AU - Osipova, E.

AU - Okuneva, E.

AU - Pakhorukov, A.

AU - Pan, A.

AU - Pankov, L.

AU - Panov, A.

AU - Rubtsov, G.

AU - Samoliga, V.

AU - Sokolov, A.

AU - Вайдянатан, Арун

N1 - Conference code: 38

PY - 2024/9/27

Y1 - 2024/9/27

N2 - This paper is devoted to the analysis of simulation results of TAIGA-IACT in stereo mode of observations and describes the technique of gamma-ray detection with energies higher than several TeV. TAIGA-IACT is part of the TAIGA astrophysics complex. Installation currently consists of three operating telescopes located 300-500 m apart. Two additional telescopes will begin operation in the next two years. We describe a new gamma-hadron separation technique for point-like source observations.

AB - This paper is devoted to the analysis of simulation results of TAIGA-IACT in stereo mode of observations and describes the technique of gamma-ray detection with energies higher than several TeV. TAIGA-IACT is part of the TAIGA astrophysics complex. Installation currently consists of three operating telescopes located 300-500 m apart. Two additional telescopes will begin operation in the next two years. We describe a new gamma-hadron separation technique for point-like source observations.

UR - https://www.scopus.com/record/display.uri?eid=2-s2.0-85212308162&origin=inward&txGid=15bdf8138f5e69093f08b81c8aac83ad

UR - https://www.mendeley.com/catalogue/dd274eeb-e681-3471-8356-2963aff6c460/

U2 - 10.22323/1.444.0686

DO - 10.22323/1.444.0686

M3 - Conference article

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

M1 - 686

T2 - 38th International Cosmic Ray Conference

Y2 - 26 July 2023 through 3 August 2023

ER -

ID: 62141411