300-800 MHz LNA-Integrated Log-Periodic Dipole Antenna for BURSTT

BURSTT (Bustling Universe Radio Survey Telescope in Taiwan) is an array antenna in Taiwan for detecting and localizing Fast Radio Bursts (FRBs). To increase its detection probability, system with wide field of view (FoV), wide bandwidth, and high sensitivity is required. To address these demands, a log-periodic dipole antenna covering 300 to 800 MHz is designed and fabricated. The antenna is with <tex xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">$\sim 8 \text{dBi}$</tex> gain and beamwidth of 60- and 90-degree for E- and H-plane, respectively. Furthermore, the LNA is placed at the feed point of the antenna to maximize the system sensitivity. Improvement was confirmed by measuring on-sky system equivalent flux density (SEFD).

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Publication Details

Published
2025-03-30
DOI
https://doi.org/10.23919/eucap63536.2025.11000028
Primary Topic
Antenna Design and Analysis
Type
article
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article

300-800 MHz LNA-Integrated Log-Periodic Dipole Antenna for BURSTT

Kai-Yang Lin, Hsien-Chun Tseng, Ue‐Li Pen, Chen Chien et al.
Antenna Design and Analysis
article

300-800 MHz LNA-Integrated Log-Periodic Dipole Antenna for BURSTT

Kai-Yang Lin, Hsien-Chun Tseng, Ue‐Li Pen, Chen Chien, Homin Jiang, Chau-Ching Chiong, Somnath Dutta, Chang-Shao Shen, Yuh-Jing Hwang, Chin-Ting Ho, Yao‐Huan Tseng, Yu-Chieh Huang, Pai-An Chen, Chao-Ching Wang, Jen‐Chieh Cheng, Chao-Te Li, Shih-Hao Wang, Shu-Hao Chang
article en

Abstract

BURSTT (Bustling Universe Radio Survey Telescope in Taiwan) is an array antenna in Taiwan for detecting and localizing Fast Radio Bursts (FRBs). To increase its detection probability, system with wide field of view (FoV), wide bandwidth, and high sensitivity is required. To address these demands, a log-periodic dipole antenna covering 300 to 800 MHz is designed and fabricated. The antenna is with <tex xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">$\sim 8 \text{dBi}$</tex> gain and beamwidth of 60- and 90-degree for E- and H-plane, respectively. Furthermore, the LNA is placed at the feed point of the antenna to maximize the system sensitivity. Improvement was confirmed by measuring on-sky system equivalent flux density (SEFD).

Institute of Astronomy and Astrophysics, Academia Sinica (TW)
Affordable and clean energy
Openalex Percentile: Top 85%
Antenna Design and Analysis
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