Author:
Tameda Yuichiro,Yamamoto Mashu,Tomida Takayuki,Ikeda Daisuke,Yamazaki Katsuya,Iwakura Hirokazu,Nakamura Yuya,Saito Yasunori
Abstract
In the future, ultra-high energy cosmic ray (UHECR) observatory will be expanded due to the small flux. Then, cost reduction is useful strategy to realize a huge scale observatory. For this purpose, we are developing a simple structure cosmic ray detector named as Cosmic Ray Air Fluorescence Fresnel-lens Telescope (CRAFFT). We deployed CRAFFT detectors at the Telescope Array site and performed a test observation. We have successfully observed UHECR air showers. We will report the status and the result of the test observation.
Cited by
1 articles.
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