Progress and future prospect of the CRAFFT project for the next generation UHECR observation

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  • <p>ICRC</p>

    ICRC

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  • uploaded June 25, 2021

Discussion timeslot (ZOOM-Meeting): 15. July 2021 - 18:00

ZOOM-Meeting URL: https://desy.zoom.us/j/92210078166

ZOOM-Meeting ID: 92210078166

ZOOM-Meeting Passcode: ICRC2021

Corresponding Session: https://icrc2021-venue.desy.de/channel/07-Where-to-go-in-UHECR-observations-CRI/123

Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-03/4

Abstract:

'Signs of anisotropy of the ultra-high-energy cosmic ray (UHECR) arrival direction have been reported by The Telescope Array and The Pierre Auger Observatory. Then, it is expected that source of UHECRs will be clarified. However, because of the quite low flux of UHECR, it is inevitable to extend observatory to much larger than existing ones. Cosmic Ray Fluorescence Fresnel lens Telescope (CRAFFT) project has been developed a low cost fluorescence detector to realize the huge observatory for UHECR observation. CRAFFT project reduced the cost to 1/10 agains fluorescence detectors now in use, and succeeded to observe UHECR air showers by the prototype of CRAFFT telescope. In this presentation, we report the progress of CRAFFT project such as the result of the test observation and data analysis and discuss the future prospect.'

Authors: Yuichiro Tameda

Co-Authors: Takayuki Tomida | Daisuke Ikeda | Katsuya Yamazaki | Takashi Kagitani | Norimichi Shibata | Eiji Nishio | Hirokazu Iwakura | Yuya Nakamura | Yuto Kubota | Shinnosuke Kurisu | Ryosuke Saito

Collaboration: CRAFFT

Indico-ID: 527

Proceeding URL: https://pos.sissa.it/395/408

Tags:
Presenter: Yuichiro Tameda

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