Orateur
Dr
Yuichiro Tameda
(Osaka Electro-Communication University)
Description
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 the test observation. We have successfully observed UHECR air showers. We will report the status and the result of the test observation.
Auteurs principaux
Dr
Yuichiro Tameda
(Osaka Electro-Communication University)
M.
Mashu Yamamoto
(Shinshu University)
Co-auteurs
Takayuki Tomida
(Shinshu University)
Dr
Daisuke Ikeda
(Earthquake Research Institute,The University of Tokyo)
Dr
Katsuya Yamazaki
(Kanagawa University)
M.
Hirokazu Iwakura
(Shinshu University)
M.
Yuya Nakamura
(Shinshu University)
Prof.
Yasunori Saito
(Shinshu University)
M.
Yuki Kaino
(Osaka Electro-Communication University)
Mlle
Yurina Ogoshi
(Osaka Electro-Communication University)
