The TAIGA timing array HiSCORE - First results

M. Tluczykont; N. Budnev; I. Astapov; N. Barbashina; A. Bogdanov; V. Boreyko; M. Brückner; A. Chiavassa; O. Chvalaev; O. Gress; T. Gress; O. Grishin; A. Dyachok; S. Epimakhov; O. Fedorov; A. Gafarov; N. Gorbunov; V. Grebenyuk; A. Grinuk; D. Horns; A. Kalinin; N. Karpov; N. Kalmykov; Y. Kazarina; S. Kiryuhin; R. Kokoulin; K. Kompaniets; A. Konstantinov; E. Korosteleva; V. Kozhin; E. Kravchenko; M. Kunnas; L. Kuzmichev; Yu Lemeshev; B. Lubsandorzhiev; N. Lubsandorzhiev; R. Mirgazov; R. Mirzoyan; R. Monkhoev; R. Nachtigall; E. Osipova; A. Pakhorukov; M. Panasyuk; L. Pankov; A. Petrukhin; V. Poleschuk; E. Popova; A. Porelli; E. Postnikov; V. Prosin; V. Ptuskin; G. Rubtsov; A. Pushnin; V. Samoliga; P. Satunin; Yu Semeney; A. Silaev; A. Silaev; A. Skurikhin; M. Slunecka; A. Sokolov; C. Spiering; L. Sveshnikova; V. Tabolenko; B. Tarashansky; A. Tkachenko; L. Tkachev; D. Voronin; R. Wischnewski; A. Zagorodnikov; V. Zurbanov; D. Zhurov; I. Yashin

doi:10.1051/epjconf/201713603008

The TAIGA timing array HiSCORE - First results

M. Tluczykont, N. Budnev, I. Astapov, N. Barbashina, A. Bogdanov, V. Boreyko, M. Brückner, A. Chiavassa, O. Chvalaev, O. Gress, T. Gress, O. Grishin, A. Dyachok, S. Epimakhov, O. Fedorov, A. Gafarov, N. Gorbunov, V. Grebenyuk, A. Grinuk, D. HornsA. Kalinin, N. Karpov, N. Kalmykov, Y. Kazarina, S. Kiryuhin, R. Kokoulin, K. Kompaniets, A. Konstantinov, E. Korosteleva, V. Kozhin, E. Kravchenko, M. Kunnas, L. Kuzmichev, Yu Lemeshev, B. Lubsandorzhiev, N. Lubsandorzhiev, R. Mirgazov, R. Mirzoyan, R. Monkhoev, R. Nachtigall, E. Osipova, A. Pakhorukov, M. Panasyuk, L. Pankov, A. Petrukhin, V. Poleschuk, E. Popova, A. Porelli, E. Postnikov, V. Prosin, V. Ptuskin, G. Rubtsov, A. Pushnin, V. Samoliga, P. Satunin, Yu Semeney, A. Silaev, A. Silaev, A. Skurikhin, M. Slunecka, A. Sokolov, C. Spiering, L. Sveshnikova, V. Tabolenko, B. Tarashansky, A. Tkachenko, L. Tkachev, D. Voronin, R. Wischnewski, A. Zagorodnikov, V. Zurbanov, D. Zhurov, I. Yashin

Результат исследования: Научные публикации в периодических изданиях › статья › рецензирование

7 Цитирования (Scopus)

Аннотация

Observations of gamma rays up to several 100 TeV are particularly important to spectrally resolve the cutoff regime of the long-sought Pevatrons, the cosmic-ray PeV accelerators. One component of the TAIGA hybrid detector is the TAIGA-HiSCORE timing array, which currently consists of 28 wide angle (0.6 sr) air Cherenkov timing stations distributed on an area of 0.25 km². The HiSCORE concept is based on (non-imaging) air shower front sampling with Cherenkov light. First results are presented.

Язык оригинала	английский
Номер статьи	03008
Число страниц	4
Журнал	EPJ Web of Conferences
Том	136
DOI	https://doi.org/10.1051/epjconf/201713603008
Состояние	Опубликовано - 23 мар. 2017

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10.1051/epjconf/201713603008

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Tluczykont, M., Budnev, N., Astapov, I., Barbashina, N., Bogdanov, A., Boreyko, V., Brückner, M., Chiavassa, A., Chvalaev, O., Gress, O., Gress, T., Grishin, O., Dyachok, A., Epimakhov, S., Fedorov, O., Gafarov, A., Gorbunov, N., Grebenyuk, V., Grinuk, A., ... Yashin, I. (2017). The TAIGA timing array HiSCORE - First results. EPJ Web of Conferences, 136, [03008]. https://doi.org/10.1051/epjconf/201713603008

@article{6f69da79f84e4b96a203c046994bdda6,

title = "The TAIGA timing array HiSCORE - First results",

abstract = "Observations of gamma rays up to several 100 TeV are particularly important to spectrally resolve the cutoff regime of the long-sought Pevatrons, the cosmic-ray PeV accelerators. One component of the TAIGA hybrid detector is the TAIGA-HiSCORE timing array, which currently consists of 28 wide angle (0.6 sr) air Cherenkov timing stations distributed on an area of 0.25 km2. The HiSCORE concept is based on (non-imaging) air shower front sampling with Cherenkov light. First results are presented.",

keywords = "GAMMA-RAY, ASTROPHYSICS",

author = "M. Tluczykont and N. Budnev and I. Astapov and N. Barbashina and A. Bogdanov and V. Boreyko and M. Br{\"u}ckner and A. Chiavassa and O. Chvalaev and O. Gress and T. Gress and O. Grishin and A. Dyachok and S. Epimakhov and O. Fedorov and A. Gafarov and N. Gorbunov and V. Grebenyuk and A. Grinuk and D. Horns and A. Kalinin and N. Karpov and N. Kalmykov and Y. Kazarina and S. Kiryuhin and R. Kokoulin and K. Kompaniets and A. Konstantinov and E. Korosteleva and V. Kozhin and E. Kravchenko and M. Kunnas and L. Kuzmichev and Yu Lemeshev and B. Lubsandorzhiev and N. Lubsandorzhiev and R. Mirgazov and R. Mirzoyan and R. Monkhoev and R. Nachtigall and E. Osipova and A. Pakhorukov and M. Panasyuk and L. Pankov and A. Petrukhin and V. Poleschuk and E. Popova and A. Porelli and E. Postnikov and V. Prosin and V. Ptuskin and G. Rubtsov and A. Pushnin and V. Samoliga and P. Satunin and Yu Semeney and A. Silaev and A. Silaev and A. Skurikhin and M. Slunecka and A. Sokolov and C. Spiering and L. Sveshnikova and V. Tabolenko and B. Tarashansky and A. Tkachenko and L. Tkachev and D. Voronin and R. Wischnewski and A. Zagorodnikov and V. Zurbanov and D. Zhurov and I. Yashin",

year = "2017",

month = mar,

day = "23",

doi = "10.1051/epjconf/201713603008",

language = "English",

volume = "136",

journal = "EPJ Web of Conferences",

issn = "2101-6275",

publisher = "EDP Sciences",

}

Tluczykont, M, Budnev, N, Astapov, I, Barbashina, N, Bogdanov, A, Boreyko, V, Brückner, M, Chiavassa, A, Chvalaev, O, Gress, O, Gress, T, Grishin, O, Dyachok, A, Epimakhov, S, Fedorov, O, Gafarov, A, Gorbunov, N, Grebenyuk, V, Grinuk, A, Horns, D, Kalinin, A, Karpov, N, Kalmykov, N, Kazarina, Y, Kiryuhin, S, Kokoulin, R, Kompaniets, K, Konstantinov, A, Korosteleva, E, Kozhin, V, Kravchenko, E, Kunnas, M, Kuzmichev, L, Lemeshev, Y, Lubsandorzhiev, B, Lubsandorzhiev, N, Mirgazov, R, Mirzoyan, R, Monkhoev, R, Nachtigall, R, Osipova, E, Pakhorukov, A, Panasyuk, M, Pankov, L, Petrukhin, A, Poleschuk, V, Popova, E, Porelli, A, Postnikov, E, Prosin, V, Ptuskin, V, Rubtsov, G, Pushnin, A, Samoliga, V, Satunin, P, Semeney, Y, Silaev, A, Silaev, A, Skurikhin, A, Slunecka, M, Sokolov, A, Spiering, C, Sveshnikova, L, Tabolenko, V, Tarashansky, B, Tkachenko, A, Tkachev, L, Voronin, D, Wischnewski, R, Zagorodnikov, A, Zurbanov, V, Zhurov, D & Yashin, I 2017, 'The TAIGA timing array HiSCORE - First results', EPJ Web of Conferences, том. 136, 03008. https://doi.org/10.1051/epjconf/201713603008

TY - JOUR

T1 - The TAIGA timing array HiSCORE - First results

AU - Tluczykont, M.

AU - Budnev, N.

AU - Astapov, I.

AU - Barbashina, N.

AU - Bogdanov, A.

AU - Boreyko, V.

AU - Brückner, M.

AU - Chiavassa, A.

AU - Chvalaev, O.

AU - Gress, O.

AU - Gress, T.

AU - Grishin, O.

AU - Dyachok, A.

AU - Epimakhov, S.

AU - Fedorov, O.

AU - Gafarov, A.

AU - Gorbunov, N.

AU - Grebenyuk, V.

AU - Grinuk, A.

AU - Horns, D.

AU - Kalinin, A.

AU - Karpov, N.

AU - Kalmykov, N.

AU - Kazarina, Y.

AU - Kiryuhin, S.

AU - Kokoulin, R.

AU - Kompaniets, K.

AU - Konstantinov, A.

AU - Korosteleva, E.

AU - Kozhin, V.

AU - Kravchenko, E.

AU - Kunnas, M.

AU - Kuzmichev, L.

AU - Lemeshev, Yu

AU - Lubsandorzhiev, B.

AU - Lubsandorzhiev, N.

AU - Mirgazov, R.

AU - Mirzoyan, R.

AU - Monkhoev, R.

AU - Nachtigall, R.

AU - Osipova, E.

AU - Pakhorukov, A.

AU - Panasyuk, M.

AU - Pankov, L.

AU - Petrukhin, A.

AU - Poleschuk, V.

AU - Popova, E.

AU - Porelli, A.

AU - Postnikov, E.

AU - Prosin, V.

AU - Ptuskin, V.

AU - Rubtsov, G.

AU - Pushnin, A.

AU - Samoliga, V.

AU - Satunin, P.

AU - Semeney, Yu

AU - Silaev, A.

AU - Skurikhin, A.

AU - Slunecka, M.

AU - Sokolov, A.

AU - Spiering, C.

AU - Sveshnikova, L.

AU - Tabolenko, V.

AU - Tarashansky, B.

AU - Tkachenko, A.

AU - Tkachev, L.

AU - Voronin, D.

AU - Wischnewski, R.

AU - Zagorodnikov, A.

AU - Zurbanov, V.

AU - Zhurov, D.

AU - Yashin, I.

PY - 2017/3/23

Y1 - 2017/3/23

N2 - Observations of gamma rays up to several 100 TeV are particularly important to spectrally resolve the cutoff regime of the long-sought Pevatrons, the cosmic-ray PeV accelerators. One component of the TAIGA hybrid detector is the TAIGA-HiSCORE timing array, which currently consists of 28 wide angle (0.6 sr) air Cherenkov timing stations distributed on an area of 0.25 km2. The HiSCORE concept is based on (non-imaging) air shower front sampling with Cherenkov light. First results are presented.

AB - Observations of gamma rays up to several 100 TeV are particularly important to spectrally resolve the cutoff regime of the long-sought Pevatrons, the cosmic-ray PeV accelerators. One component of the TAIGA hybrid detector is the TAIGA-HiSCORE timing array, which currently consists of 28 wide angle (0.6 sr) air Cherenkov timing stations distributed on an area of 0.25 km2. The HiSCORE concept is based on (non-imaging) air shower front sampling with Cherenkov light. First results are presented.

KW - GAMMA-RAY

KW - ASTROPHYSICS

UR - http://www.scopus.com/inward/record.url?scp=85017139251&partnerID=8YFLogxK

U2 - 10.1051/epjconf/201713603008

DO - 10.1051/epjconf/201713603008

M3 - Article

AN - SCOPUS:85017139251

VL - 136

JO - EPJ Web of Conferences

JF - EPJ Web of Conferences

SN - 2101-6275

M1 - 03008

ER -

The TAIGA timing array HiSCORE - First results

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