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TAIGA-HiSCORE : Results from the first two operation seasons. / the TAIGA Collaboration.

In: Proceedings of Science, Vol. Part F135186, 01.01.2017.

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

Harvard

the TAIGA Collaboration 2017, 'TAIGA-HiSCORE: Results from the first two operation seasons', Proceedings of Science, vol. Part F135186.

APA

the TAIGA Collaboration (2017). TAIGA-HiSCORE: Results from the first two operation seasons. Proceedings of Science, Part F135186.

Vancouver

the TAIGA Collaboration. TAIGA-HiSCORE: Results from the first two operation seasons. Proceedings of Science. 2017 Jan 1;Part F135186.

Author

the TAIGA Collaboration. / TAIGA-HiSCORE : Results from the first two operation seasons. In: Proceedings of Science. 2017 ; Vol. Part F135186.

BibTeX

@article{6f063328605845d4966f2a81dddf99bc,
title = "TAIGA-HiSCORE: Results from the first two operation seasons",
abstract = "The very to ultra high energy gamma-ray regime up to several 100 TeV is the key to spectrally resolve the cutoff regime of the long-sought Pevatrons, the Galactic cosmic-ray PeV accelerators. One component of the TAIGA hybrid detector is the TAIGA-HiSCORE shower-front sampling timing array, which currently consists of 28 wide angle (0.6 sr) air Cherenkov timing stations distributed on an area of 0.25 km2, and which will be doubled in area by fall 2017. We report on the status and first results of the HiSCORE timing array after the first two operation seasons, including calibration studies on timing and pointing, cross calibration with data from the first TAIGA-IACT, observations with the timing array of a LIDAR operating on the ISS, a measurement of the Cosmic Ray spectrum, and a search for high energy gamma-rays from Galactic sources such as the Crab Nebula.",
author = "{the TAIGA Collaboration} and M. Tluczykont and O. Gress and E. Korosteleva and L. Kuzmichev and A. Pakhorukov and A. Porelli and V. Prosin and L. Sveshnikova and R. Wischnewski and I. Astapov and P. Bezyazeekov and V. Boreyko and A. Borodin and M. Brueckner and N. Budnev and A. Chiavassa and A. Dyachok and O. Fedorov and A. Gafarov and A. Garmash and N. Gorbunov and V. Grebenyuk and T. Gress and O. Grishin and A. Grinyuk and D. Horns and A. Ivanova and N. Kalmykov and Y. Kazarina and V. Kindin and P. Kirilenko and S. Kiryuhin and R. Kokoulin and K. Kompaniets and V. Kozhin and E. Kravchenko and M. Kunnas and Yu Lemeshev and V. Lenok and B. Lubsandorzhiev and N. Lubsandorzhiev and R. Mirgazov and R. Mirzoyan and R. Monkhoev and R. Nachtigall and E. Osipova and M. Panasyuk and L. Pankov and A. Petrukhin and A. Sokolov",
year = "2017",
month = jan,
day = "1",
language = "English",
volume = "Part F135186",
journal = "Proceedings of Science",
issn = "1824-8039",
publisher = "Sissa Medialab Srl",
note = "35th International Cosmic Ray Conference, ICRC 2017 ; Conference date: 10-07-2017 Through 20-07-2017",

}

RIS

TY - JOUR

T1 - TAIGA-HiSCORE

T2 - 35th International Cosmic Ray Conference, ICRC 2017

AU - the TAIGA Collaboration

AU - Tluczykont, M.

AU - Gress, O.

AU - Korosteleva, E.

AU - Kuzmichev, L.

AU - Pakhorukov, A.

AU - Porelli, A.

AU - Prosin, V.

AU - Sveshnikova, L.

AU - Wischnewski, R.

AU - Astapov, I.

AU - Bezyazeekov, P.

AU - Boreyko, V.

AU - Borodin, A.

AU - Brueckner, M.

AU - Budnev, N.

AU - Chiavassa, A.

AU - Dyachok, A.

AU - Fedorov, O.

AU - Gafarov, A.

AU - Garmash, A.

AU - Gorbunov, N.

AU - Grebenyuk, V.

AU - Gress, T.

AU - Grishin, O.

AU - Grinyuk, A.

AU - Horns, D.

AU - Ivanova, A.

AU - Kalmykov, N.

AU - Kazarina, Y.

AU - Kindin, V.

AU - Kirilenko, P.

AU - Kiryuhin, S.

AU - Kokoulin, R.

AU - Kompaniets, K.

AU - Kozhin, V.

AU - Kravchenko, E.

AU - Kunnas, M.

AU - Lemeshev, Yu

AU - Lenok, V.

AU - Lubsandorzhiev, B.

AU - Lubsandorzhiev, N.

AU - Mirgazov, R.

AU - Mirzoyan, R.

AU - Monkhoev, R.

AU - Nachtigall, R.

AU - Osipova, E.

AU - Panasyuk, M.

AU - Pankov, L.

AU - Petrukhin, A.

AU - Sokolov, A.

PY - 2017/1/1

Y1 - 2017/1/1

N2 - The very to ultra high energy gamma-ray regime up to several 100 TeV is the key to spectrally resolve the cutoff regime of the long-sought Pevatrons, the Galactic cosmic-ray PeV accelerators. One component of the TAIGA hybrid detector is the TAIGA-HiSCORE shower-front sampling timing array, which currently consists of 28 wide angle (0.6 sr) air Cherenkov timing stations distributed on an area of 0.25 km2, and which will be doubled in area by fall 2017. We report on the status and first results of the HiSCORE timing array after the first two operation seasons, including calibration studies on timing and pointing, cross calibration with data from the first TAIGA-IACT, observations with the timing array of a LIDAR operating on the ISS, a measurement of the Cosmic Ray spectrum, and a search for high energy gamma-rays from Galactic sources such as the Crab Nebula.

AB - The very to ultra high energy gamma-ray regime up to several 100 TeV is the key to spectrally resolve the cutoff regime of the long-sought Pevatrons, the Galactic cosmic-ray PeV accelerators. One component of the TAIGA hybrid detector is the TAIGA-HiSCORE shower-front sampling timing array, which currently consists of 28 wide angle (0.6 sr) air Cherenkov timing stations distributed on an area of 0.25 km2, and which will be doubled in area by fall 2017. We report on the status and first results of the HiSCORE timing array after the first two operation seasons, including calibration studies on timing and pointing, cross calibration with data from the first TAIGA-IACT, observations with the timing array of a LIDAR operating on the ISS, a measurement of the Cosmic Ray spectrum, and a search for high energy gamma-rays from Galactic sources such as the Crab Nebula.

UR - http://www.scopus.com/inward/record.url?scp=85046053760&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:85046053760

VL - Part F135186

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

Y2 - 10 July 2017 through 20 July 2017

ER -

ID: 12563302