| Title: | TA SD analysis for inclined air showers |
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| Authors: | ID Takahashi, K. (Author)
ID Lundquist, Jon Paul (Author), et al. |
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| Files: |  ICRC2023_306.pdf (1,13 MB)
MD5: B06E92C3ECD35385211E774416C2F2A9
 https://pos.sissa.it/444/306/
https://pos.sissa.it/444/306/pdf
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| Language: | English |
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| Work type: | Not categorized |
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| Typology: | 1.08 - Published Scientific Conference Contribution |
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| Organization: | UNG - University of Nova Gorica
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| Abstract: | The origin of UHECRs is an open question which is complicated due to not very well-known deflections of the charged particles in Galactic and intergalactic magnetic fields. Finding the EeV neutrinos from astronomical sources will be a key to solve the problem of the origin. EeV neutrinos are expected to produce extensive air showers which are observable by the current operational air shower arrays. To search for neutrino-induced showers, it is important to increase both the interaction probability and background rejection power in the analysis of the inclined showers. We study a reconstruction method of the Telescope Array surface detector (TA SD) data for the neutrino-induced inclined air showers. The prime target is to improve the angular resolution for the astronomical objects. In this contribution, we present the detail of analysis method, angular resolution and total exposure of TA SD for neutrinos from the astronomical objects as a function of the declination. |
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| Keywords: | Telescope Array, indirect detection, surface detection, ground array, ultra-high energy, cosmic rays, inclined showers, neutrinos |
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| Publication status: | Submitted to the publisher |
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| Year of publishing: | 2023 |
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| PID: | 20.500.12556/RUNG-8560  |
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| COBISS.SI-ID: | 167663875 |
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| DOI: | 10.22323/1.444.0306 |
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| NUK URN: | URN:SI:UNG:REP:FA28MB96 |
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| Publication date in RUNG: | 09.10.2023 |
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| Views: | 1861 |
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| Downloads: | 6 |
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