| Naslov: | Current status and prospects of surface detector of the TAx4 experiment |
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| Avtorji: | ID Kido, E. (Avtor)
ID Lundquist, Jon Paul (Avtor), et al. |
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| Datoteke: |  ICRC2021_203.pdf (1,30 MB)
MD5: F23850D7FD584276EF78E9C86579EF3C
 https://pos.sissa.it/395/203/
https://pos.sissa.it/395/203/pdf
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| Jezik: | Angleški jezik |
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| Vrsta gradiva: | Delo ni kategorizirano |
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| Tipologija: | 1.08 - Objavljeni znanstveni prispevek na konferenci |
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| Organizacija: | UNG - Univerza v Novi Gorici
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| Opis: | Telescope Array (TA) is the largest ultrahigh energy cosmic-ray (UHECR) observatory in the Northern Hemisphere. A surface detector (SD) array covers approximately 700 km^2, and the SD array is surrounded by three fluorescence detector (FD) stations. TA has found evidence for a cluster of cosmic rays with energies greater than 57 EeV from the TA SD data. In order to confirm this evidence with more data, we started the TAx4 experiment which expands the detection area using new SDs and FDs. We started construction of new SDs which are arranged in a square grid with 2.08 km spacing at the north east and south east of the TA SD array. More than half of the new SDs are already deployed and running. We present the current status of the TAx4 SD, trigger efficiency and exposure prospects for the highest energy part of the cosmic ray spectrum. |
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| Ključne besede: | Telescope Array, TAx4, indirect detection, surface detection, ground array, ultra-high energy, cosmic rays, trigger efficiency |
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| Status publikacije: | Objavljeno |
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| Leto izida: | 2022 |
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| PID: | 20.500.12556/RUNG-8543  |
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| COBISS.SI-ID: | 167055875 |
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| DOI: | 10.22323/1.395.0203 |
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| NUK URN: | URN:SI:UNG:REP:W22VJMUW |
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| Datum objave v RUNG: | 04.10.2023 |
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| Število ogledov: | 1885 |
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| Število prenosov: | 10 |
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| Metapodatki: |    |
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