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- W4387133635 abstract "The ALPACA experiment is a project aiming to observe sub-PeV gamma rays for the first time in the southern hemisphere. The main goal of ALPACA is to identify PeVatrons, the accelerators of Galactic PeV cosmic rays, by observing sub-PeV pion-decay gamma rays generated in interactions between PeV cosmic rays and the interstellar medium. This new air shower experiment is located at an altitude of 4,740 m above sea level in the middle of Mt. Chacaltaya in Bolivia. The air shower array consists of 401 scintillation counters covering an 83,000 m ^2 <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:msup><mml:mi /><mml:mn>2</mml:mn></mml:msup></mml:math> surface area. In addition, a water-Cherenkov-type muon detector array with an area of 3,700 m ^2 <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:msup><mml:mi /><mml:mn>2</mml:mn></mml:msup></mml:math> is installed to discriminate gamma rays from background cosmic rays. The prototype array ALPAQUITA will start data taking in 2022 and will extend to ALPACA in 2024. We report on a general introduction to ALPACA, the progress of the project, and the sensitivity to sub-PeV gamma rays." @default.
- W4387133635 created "2023-09-29" @default.
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- W4387133635 date "2023-09-28" @default.
- W4387133635 modified "2023-10-18" @default.
- W4387133635 title "The ALPACA experiment: The project of the first sub-PeV gamma-ray observation in the southern sky" @default.
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- W4387133635 doi "https://doi.org/10.21468/scipostphysproc.13.008" @default.
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