12–23 Jul 2021
Online
Europe/Berlin timezone

Progress in optimizing the detection surface structure of CRAFFT

21 Jul 2021, 12:00
1h 30m
03

03

Poster CRI | Cosmic Ray Indirect Discussion

Speaker

Yuto Kubota (Shinshu university)

Description

A observatory for the next generation of ultra-high energy cosmic rays (UHECRs) should be expanded for clarifying the origin and nature of UHECRs. In order to realize a huge UHECR observatory, we are developing Cosmic Ray Air Fluorescence Fresnel lens Telescope (CRAFFT), which is a low-cost fluorescence telescope.We tested a performance of prototype CRAFFT at Telescope Array (TA) site, and succeeded to detect UHECR air showers synchronized with TA detectors in 2017.We are currently developing a reconstruction method based on waveform fitting with sufficient analysis accuracy, and optimizing the detector configuration to improve its performance with low cost.Progress in detector optimization, reconstruction method, and calibrations such as uniformity of PMT sensitivity will be discussed.

Keywords

UHECR, fluorescence telescope, fresnel lens, development,

Subcategory Experimental Methods & Instrumentation
Collaboration other (fill field below)
other Collaboration CRAFFT

Primary author

Yuto Kubota (Shinshu university)

Co-authors

Daisuke Ikeda (Kanagawa University) Mr Takashi Kagitani (Osaka Electro-Communication University) Takayuki Tomida (Shinshu University) Yuichiro Tameda (Osaka Electro-Communication University) Mr Norimichi Shibata (Osaka Electro-Communication University) for the CRAFFT Collaboration

Presentation materials