3–7 Oct 2022
Gran Sasso Science Institute, L'Aquila, Italy
Europe/Rome timezone

Current status of the TAx4 surface detectors

4 Oct 2022, 16:30
20m
Gran Sasso Science Institute, L'Aquila, Italy

Gran Sasso Science Institute, L'Aquila, Italy

Via Michele Iacobucci, 2 L'Aquila, Italy
Talk

Speaker

Dr Eiji Kido (RIKEN, Cluster for Pioneering Research)

Description

Telescope Array (TA) is the largest ultrahigh-energy cosmic-ray (UHECR) observatory in the northern hemisphere. It explores the origin of UHECRs using a surface detector (SD) array covering approximately 700 km$^2$ and fluorescence detector (FD) stations. TA has found evidence for a cluster of cosmic rays with energies greater than 57 EeV known as a hotspot. Recently, implications of anisotropy in the arrival directions in other energy ranges were obtained. Implications of spectrum anisotropy were also obtained. The new SD array of the TAx4 experiment was designed to increase the data collection rate at the highest energies to confirm the implications with more data. We constructed more than half SDs of the TAx4 experiment and have stably operated the SDs. We present TAx4 SD’s current status and the data that have already been collected.

Primary author

Dr Eiji Kido (RIKEN, Cluster for Pioneering Research)

Presentation materials