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Commissioning the joint operation of the wide angle timing HiSCORE Cherenkov array with the first IACT of the TAIGA experimenдоклад на конференции
- Авторы: Boreyko V., Bezyazeekov P., Brueckner M., Sveshnikova L., Astapov I., Chiavassa N.Budnev A, Dyachok A., Fedorov O., Gafarov A., Gorbunov N., Grebenyuk V., Gress O., Gress T., Grishin O., Grinyuk A., Horns D., Ivanova A., Kalmykov N., Kazarina Y., Kindin V., Kiryuhin S., Kokoulin R., Kompaniets K., Korosteleva E., Kozhin V., Kravchenko E., Kunnas M., Kuzmichev L., Lemeshev Yu, Lenok V., Lubsandorzhiev B., Lubsandorzhie N., Mirgazov R., Mirzoyan R., Monkhoev R., Nachtigal R., Osipova E., Pakhorukov A., Panasyuk M., Pankov L., Postnikov E.B., Popova E.G., Borodin A.
- Международная Конференция : 35th International Cosmic Ray Conference
- Даты проведения конференции: 12-20 июля 2017
- Дата доклада: 13 июля 2017
- Тип доклада: Стендовый
- Докладчик: не указан
- Место проведения: Busan, Korea, Republic of
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Аннотация доклада:
The first IACT as part of the gamma and cosmic-ray experiment TAIGA was installed in the Tunka valley near lake Baikal in fall 2016. In the following months different systems of the telescope were put into test operation. We started the commissioning phase of operating the telescope in time coincidence with the wide angle integrating air Cherenkov HiSCORE array, which for the time being comprises 28 operational stations. We anticipate that the hybrid operation of the non-imaging and imaging telescopes will lead to a cost-efficient, highly sensitive detector operating in the energy range from 30-50 TeV till several PeV. Here we want to report on the first test results of operating the prototype hybrid array. We will focus on the analysis of background cosmic ray flux, count rates, energy and angular resolutions, shower core position reconstruction for coincident events, comparing these with expectations from MC simulations.
- Добавил в систему: Свешникова Любовь Георгиевна