Design and Commissioning of the BURSTT-256 Main Antenna Array for the Fast Radio Burst Survey in the Local Universe
Abstract
The Bustling Universe Radio Survey Telescope in Taiwan (BURSTT) is a radio interferometer array designed for surveying fast radio bursts (FRBs) in the nearby Universe with a wide instantaneous field of view (FoV) of ≈6000 deg2 and precisely localizing them with sub-arcsecond angular resolution. The first phase of BURSTT, BURSTT-256, consists of a main antenna array comprising 256 log-periodic dipole antennas (LPDAs) observing at 400-800 MHz for real-time beamforming and FRB search, currently with 256 beams covering ≈ 3200 deg2 FoV, together with several smaller outrigger stations with 16-64 antennas and separated by 𝒪(102 − 103) km baselines for joint observations to localize FRBs using very-long baseline interferometry. This work presents the design, deployment, and commissioning of the BURSTT-256 main array, including site selection, radio-frequency (RF) background characterization, receiver antenna array and RF front-end, as well as real-time, factorized digital beamforming backend that currently generates 256 beams. The system's on-sky performance, sensitivity, and beamforming fidelity have been calibrated through observations of bright celestial calibrators. The antenna array in the initial phase using commercial LPDAs has a system equivalent flux density of ≈11 kJy, and is expected to achieve ≈4 kJy using custom-design LPDAs after optimization in late 2026. BURSTT-256 serves as a critical pathfinder for future expansion of the array to 2048 elements and beyond, operating at 300-700 MHz with ≈6000 deg2 FoV. It establishes the framework required to discover and localize nearby FRBs with sub-arcsecond precision. By substantially increasing the number of well-localized nearby FRBs, BURSTT will facilitate multi-wavelength and multi-messenger counterpart identification, helping to unveil the elusive origin of FRBs.
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BibTeX
@misc{wang2026design,
title = {{Design and Commissioning of the BURSTT-256 Main Antenna Array for the Fast Radio Burst Survey in the Local Universe}},
author = {Shih-Hao Wang and Kai-Yang Lin and Chao-Te Li and Chau-Ching Chiong and Jen-Chieh Cheng and Chung-Cheng Chen and Hsien-Chun Tseng and Shu-Hao Chang and Pai-An Chen and Ta-Shun Wei and Chin-Ting Ho and Vigo Feng-Shun Wu and Yu-Chieh Huang and Sujin Eie and Yao-Huan Tseng and Ue-Li Pen and Chih-Yi Wen and Homin Jiang and Andrew Wang and Bishnu Kumar Sharma and Tzu-Hong Chen Lin and Yuan-Wei Hu and Shih-Wen Chung and Chen-Hui Peng and Ming-Tang Chen and Pisin Chen and Jiwoo Nam and Tomotsugu Goto and Tetsuya Hashimoto and Chin-Ping Hu and Yuan-Chang Hou and Daniel Baker and Michael Chiang and Somnath Dutta and Sun-Kun King and Hiroto Masaoka and Chung-Yun Kuo and Che-Wei Pai and Decmend Fang-Jie Ling},
howpublished = {arXiv},
year = {2026},
month = nov,
doi = {10.48550/arxiv.2611.07832},
eprint = {2611.07832},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2611.07832},
}
RIS
TY - UNPB
TI - Design and Commissioning of the BURSTT-256 Main Antenna Array for the Fast Radio Burst Survey in the Local Universe
AU - Shih-Hao Wang
AU - Kai-Yang Lin
AU - Chao-Te Li
AU - Chau-Ching Chiong
AU - Jen-Chieh Cheng
AU - Chung-Cheng Chen
AU - Hsien-Chun Tseng
AU - Shu-Hao Chang
AU - Pai-An Chen
AU - Ta-Shun Wei
AU - Chin-Ting Ho
AU - Vigo Feng-Shun Wu
AU - Yu-Chieh Huang
AU - Sujin Eie
AU - Yao-Huan Tseng
AU - Ue-Li Pen
AU - Chih-Yi Wen
AU - Homin Jiang
AU - Andrew Wang
AU - Bishnu Kumar Sharma
AU - Tzu-Hong Chen Lin
AU - Yuan-Wei Hu
AU - Shih-Wen Chung
AU - Chen-Hui Peng
AU - Ming-Tang Chen
AU - Pisin Chen
AU - Jiwoo Nam
AU - Tomotsugu Goto
AU - Tetsuya Hashimoto
AU - Chin-Ping Hu
AU - Yuan-Chang Hou
AU - Daniel Baker
AU - Michael Chiang
AU - Somnath Dutta
AU - Sun-Kun King
AU - Hiroto Masaoka
AU - Chung-Yun Kuo
AU - Che-Wei Pai
AU - Decmend Fang-Jie Ling
PY - 2026
DA - 2026/11/05
PB - arXiv
DO - 10.48550/arxiv.2611.07832
UR - https://arxiv.org/abs/2611.07832
AB - The Bustling Universe Radio Survey Telescope in Taiwan (BURSTT) is a radio interferometer array designed for surveying fast radio bursts (FRBs) in the nearby Universe with a wide instantaneous field of view (FoV) of ≈6000 deg^2 and precisely localizing them with sub-arcsecond angular resolution. The first phase of BURSTT, BURSTT-256, consists of a main antenna array comprising 256 log-periodic dipole antennas (LPDAs) observing at 400-800 MHz for real-time beamforming and FRB search, currently with 256 beams covering ≈ 3200 deg^2 FoV, together with several smaller outrigger stations with 16-64 antennas and separated by 𝒪(10^2 − 10^3) km baselines for joint observations to localize FRBs using very-long baseline interferometry. This work presents the design, deployment, and commissioning of the BURSTT-256 main array, including site selection, radio-frequency (RF) background characterization, receiver antenna array and RF front-end, as well as real-time, factorized digital beamforming backend that currently generates 256 beams. The system's on-sky performance, sensitivity, and beamforming fidelity have been calibrated through observations of bright celestial calibrators. The antenna array in the initial phase using commercial LPDAs has a system equivalent flux density of ≈11 kJy, and is expected to achieve ≈4 kJy using custom-design LPDAs after optimization in late 2026. BURSTT-256 serves as a critical pathfinder for future expansion of the array to 2048 elements and beyond, operating at 300-700 MHz with ≈6000 deg^2 FoV. It establishes the framework required to discover and localize nearby FRBs with sub-arcsecond precision. By substantially increasing the number of well-localized nearby FRBs, BURSTT will facilitate multi-wavelength and multi-messenger counterpart identification, helping to unveil the elusive origin of FRBs.
ER -