| Issue |
EPJ Web Conf.
Volume 210, 2019
Ultra High Energy Cosmic Rays 2018 (UHECR 2018)
|
|
|---|---|---|
| Article Number | 06001 | |
| Number of page(s) | 3 | |
| Section | Futur Detectors | |
| DOI | https://doi.org/10.1051/epjconf/201921006001 | |
| Published online | 17 May 2019 | |
https://doi.org/10.1051/epjconf/201921006001
Status and prospects of the TAx4 experiment
Institute for Cosmic Ray Research, University of Tokyo, 5-1-5 Kashiwanoha, Chiba 277-8582, Japan
* e-mail: ekido@icrr.u-tokyo.ac.jp
Published online: 17 May 2019
The TAx4 experiment is a project to observe highest energy cosmic rays by expanding the detection area of the TA experiment with newly constructed surface detectors (SDs) and fluorescence detectors (FDs). The construction of both SDs and FDs is ongoing. New SDs are arranged in a square grid with 2.08 km spacing at the north east and south east of the TA SD array. Field of view of new FDs overlaps the detection area of new SDs to observe SD FD hybrid events. New SDs are planning to be deployed early next year. The first light with new FDs was already observed on February 2018. Especially the hotspot and energy spectrum anisotropy are expected to be understood in more detail from the implications obtained by the TA experiment.
© The Authors, published by EDP Sciences, 2019
This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.