BURSTT: Bustling Universe Radio Survey Telescope in Taiwan

TL;DR

BURSTT is a new radio telescope in Taiwan designed to detect, localize, and study fast radio bursts (FRBs) with high precision, aiming to improve understanding of their origins through large-scale, continuous sky surveys.

Contribution

This paper introduces BURSTT, a novel radio telescope optimized for high-fluence FRB detection and localization, with plans to expand its antenna array for enhanced capabilities.

Findings

BURSTT-256 expected to detect ~100 bright FRBs annually.

Large FoV enables continuous monitoring and potential detection of repeating FRBs.

Sub-arcsecond localization improves source identification.

Abstract

Fast Radio Bursts (FRBs) are bright millisecond-duration radio transients that appear about 1,000 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 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, nearby FRBs. This is the population most amenable to multi-messenger, multi-wavelength follow-up, allowing deeper understanding of source mechanisms. BURSTT will provide horizon-to-horizon sky coverage with a half power field-of-view (FoV) of $\sim$10$^{4}$ deg$^{2}$, a 400 MHz effective bandwidth between 300-800 MHz, and sub-arcsecond localization, made possible using outrigger stations hundreds to thousands of km from the main array. Initially, BURSTT will employ 256 antennas. After tests of various antenna designs and optimization of system performance we plan to expand to 2048 antennas. We estimate that BURSTT-256 will detect and localize $\sim$100 bright ($\geq$100 Jy ms) FRBs per year. Another advantage of BURSTT's large FoV and continuous operation will be 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.