Progress of the GRANDProto300 Project
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arXiv
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| Format: | Preprint |
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2025
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| _version_ | 1866918086411550720 |
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| author | Ma, Pengxiong Zhang, Yi Xu, Xing Duan, Bohao Wang, Shen Zhang, Kewen Zhang, Pengfei Xu, Xin |
| author_facet | Ma, Pengxiong Zhang, Yi Xu, Xing Duan, Bohao Wang, Shen Zhang, Kewen Zhang, Pengfei Xu, Xin |
| contents | GRANDProto300 (hereafter referred to as GP300) is a pioneering prototype array of the GRAND experiment. It consists of 300 radio antennas and will cover an area of 200 km$^2$ in a radio-quiet region of western China. Serving as a test bench for the GRAND experiment, GRANDProto300 aims to achieve autonomous radio detection and reconstruction of highly inclined air showers. It is designed to detect ultra-high-energy cosmic rays in the energy range of $10^{16.5}$-$10^{18}$ eV at a rate comparable to that of the Pierre Auger Observatory. Over the past two years, significant improvements have been made to both the hardware and firmware of GP300. Currently, 65 antenna units have been deployed at the site by June 2025. We present the current status of detector commissioning, including updates on hardware, calibration results such as GPS timing and antenna positioning. Additionally, we discuss the solar radio bursts associated with solar flares, the galactic radio emissions detected, and preliminary cosmic ray surveys. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2507_05915 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Progress of the GRANDProto300 Project Ma, Pengxiong Zhang, Yi Xu, Xing Duan, Bohao Wang, Shen Zhang, Kewen Zhang, Pengfei Xu, Xin High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics High Energy Physics - Experiment High Energy Physics - Phenomenology GRANDProto300 (hereafter referred to as GP300) is a pioneering prototype array of the GRAND experiment. It consists of 300 radio antennas and will cover an area of 200 km$^2$ in a radio-quiet region of western China. Serving as a test bench for the GRAND experiment, GRANDProto300 aims to achieve autonomous radio detection and reconstruction of highly inclined air showers. It is designed to detect ultra-high-energy cosmic rays in the energy range of $10^{16.5}$-$10^{18}$ eV at a rate comparable to that of the Pierre Auger Observatory. Over the past two years, significant improvements have been made to both the hardware and firmware of GP300. Currently, 65 antenna units have been deployed at the site by June 2025. We present the current status of detector commissioning, including updates on hardware, calibration results such as GPS timing and antenna positioning. Additionally, we discuss the solar radio bursts associated with solar flares, the galactic radio emissions detected, and preliminary cosmic ray surveys. |
| title | Progress of the GRANDProto300 Project |
| topic | High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics High Energy Physics - Experiment High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2507.05915 |