BURSTT: Bustling Universe Radio Survey Telescope in Taiwan

Fast Radio Bursts (FRBs) are bright millisecond-duration radio transients that appear about 1000 times per day, all-sky, for a fluence threshold 5 Jy ms at 600 MHz. The FRB radio-emission physics and the compact objects involved in these events are subjects of intense and active debate. To better co...

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Published inPublications of the Astronomical Society of the Pacific Vol. 134; no. 1039; pp. 94106 - 94119
Main Authors Lin, Hsiu-Hsien, Lin, Kai-yang, Li, Chao-Te, Tseng, Yao-Huan, Jiang, Homin, Wang, Jen-Hung, Cheng, Jen-Chieh, Pen, Ue-Li, Chen, Ming-Tang, Chen, Pisin, Chen, Yaocheng, Goto, Tomotsugu, Hashimoto, Tetsuya, Hwang, Yuh-Jing, King, Sun-Kun, Kubo, Derek, Kuo, Chung-Yun, Mills, Adam, Nam, Jiwoo, Oshiro, Peter, Shen, Chang-Shao, Tseng, Hsien-Chun, Wang, Shih-Hao, Wu, Vigo Feng-Shun, Bower, Geoffrey, Chang, Shu-Hao, Chen, Pai-An, Chen, Ying-Chih, Chiang, Yi-Kuan, Fedynitch, Anatoli, Gusinskaia, Nina, Ho, Simon C.-C., Hsiao, Tiger Y.-Y., Hu, Chin-Ping, Huang, Yau De, Jáuregui García, José Miguel, Kim, Seong Jin, Kuo, Cheng-Yu, Ling, Decmend Fang-Jie, On, Alvina Y. L., Peterson, Jeffrey B., R. Raquel, Bjorn Jasper, Su, Shih-Chieh, Uno, Yuri, Wu, Cossas K.-W., Yamasaki, Shotaro, Zhu, Hong-Ming
Format Journal Article
LanguageEnglish
Published Philadelphia The Astronomical Society of the Pacific 01.09.2022
IOP Publishing
Subjects
Antennas
Astronomical instrumentation
Radio transient sources
Universe
Very long baseline interferometry
Wide-field telescopes
Taiwan
Online AccessGet full text
ISSN0004-6280
1538-3873
1538-3873
DOI10.1088/1538-3873/ac8f71

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Abstract Fast Radio Bursts (FRBs) are bright millisecond-duration radio transients that appear about 1000 times per day, all-sky, for a fluence threshold 5 Jy ms at 600 MHz. The FRB radio-emission physics and the compact objects involved in these events are subjects of intense and active debate. To better constrain source models, the Bustling Universe Radio Survey Telescope in Taiwan (BURSTT) is optimized to discover and localize a large sample of rare, high-fluence, and nearby FRBs. This population is the most amenable to multi-messenger and multi-wavelength follow-up, which allows a deeper understanding of source mechanisms. BURSTT will provide horizon-to-horizon sky coverage with a half power field-of-view (FoV) of ∼10 4 deg 2 , a 400 MHz effective bandwidth between 300 and 800 MHz, and subarcsecond localization, which is made possible using outrigger stations that are hundreds to thousands of km from the main array. Initially, BURSTT will employ 256 antennas. After tests of various antenna designs and optimizing the system’s performance, we plan to expand to 2048 antennas. We estimate that BURSTT-256 will detect and localize ∼100 bright (≥100 Jy ms) FRBs per year. Another advantage of BURSTT’s large FoV and continuous operation will be its greatly enhanced monitoring of FRBs for repetition. The current lack of sensitive all-sky observations likely means that many repeating FRBs are currently cataloged as single-event FRBs.
AbstractList Fast Radio Bursts (FRBs) are bright millisecond-duration radio transients that appear about 1000 times per day, all-sky, for a fluence threshold 5 Jy ms at 600 MHz. The FRB radio-emission physics and the compact objects involved in these events are subjects of intense and active debate. To better constrain source models, the Bustling Universe Radio Survey Telescope in Taiwan (BURSTT) is optimized to discover and localize a large sample of rare, high-fluence, and nearby FRBs. This population is the most amenable to multi-messenger and multi-wavelength follow-up, which allows a deeper understanding of source mechanisms. BURSTT will provide horizon-to-horizon sky coverage with a half power field-of-view (FoV) of ∼104 deg2, a 400 MHz effective bandwidth between 300 and 800 MHz, and subarcsecond localization, which is made possible using outrigger stations that are hundreds to thousands of km from the main array. Initially, BURSTT will employ 256 antennas. After tests of various antenna designs and optimizing the system’s performance, we plan to expand to 2048 antennas. We estimate that BURSTT-256 will detect and localize ∼100 bright (≥100 Jy ms) FRBs per year. Another advantage of BURSTT’s large FoV and continuous operation will be its greatly enhanced monitoring of FRBs for repetition. The current lack of sensitive all-sky observations likely means that many repeating FRBs are currently cataloged as single-event FRBs.
Fast Radio Bursts (FRBs) are bright millisecond-duration radio transients that appear about 1000 times per day, all-sky, for a fluence threshold 5 Jy ms at 600 MHz. The FRB radio-emission physics and the compact objects involved in these events are subjects of intense and active debate. To better constrain source models, the Bustling Universe Radio Survey Telescope in Taiwan (BURSTT) is optimized to discover and localize a large sample of rare, high-fluence, and nearby FRBs. This population is the most amenable to multi-messenger and multi-wavelength follow-up, which allows a deeper understanding of source mechanisms. BURSTT will provide horizon-to-horizon sky coverage with a half power field-of-view (FoV) of ∼10 4 deg 2 , a 400 MHz effective bandwidth between 300 and 800 MHz, and subarcsecond localization, which is made possible using outrigger stations that are hundreds to thousands of km from the main array. Initially, BURSTT will employ 256 antennas. After tests of various antenna designs and optimizing the system’s performance, we plan to expand to 2048 antennas. We estimate that BURSTT-256 will detect and localize ∼100 bright (≥100 Jy ms) FRBs per year. Another advantage of BURSTT’s large FoV and continuous operation will be its greatly enhanced monitoring of FRBs for repetition. The current lack of sensitive all-sky observations likely means that many repeating FRBs are currently cataloged as single-event FRBs.
Author Lin, Hsiu-Hsien
Wang, Shih-Hao
Kuo, Chung-Yun
Lin, Kai-yang
Hwang, Yuh-Jing
Chiang, Yi-Kuan
Li, Chao-Te
Chen, Pisin
Nam, Jiwoo
Cheng, Jen-Chieh
Shen, Chang-Shao
Jiang, Homin
R. Raquel, Bjorn Jasper
Tseng, Yao-Huan
On, Alvina Y. L.
King, Sun-Kun
Kuo, Cheng-Yu
Oshiro, Peter
Hsiao, Tiger Y.-Y.
Wu, Vigo Feng-Shun
Zhu, Hong-Ming
Hashimoto, Tetsuya
Goto, Tomotsugu
Peterson, Jeffrey B.
Chen, Ying-Chih
Wang, Jen-Hung
Bower, Geoffrey
Kim, Seong Jin
Huang, Yau De
Fedynitch, Anatoli
Jáuregui García, José Miguel
Tseng, Hsien-Chun
Chen, Pai-An
Yamasaki, Shotaro
Kubo, Derek
Uno, Yuri
Mills, Adam
Su, Shih-Chieh
Chen, Ming-Tang
Pen, Ue-Li
Chang, Shu-Hao
Chen, Yaocheng
Ling, Decmend Fang-Jie
Hu, Chin-Ping
Gusinskaia, Nina
Ho, Simon C.-C.
Wu, Cossas K.-W.
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SubjectTerms Antennas
Astronomical instrumentation
Radio transient sources
Universe
Very long baseline interferometry
Wide-field telescopes
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