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Record W4297215909 · doi:10.1088/1538-3873/ac8f71

BURSTT: Bustling Universe Radio Survey Telescope in Taiwan

2022· article· en· W4297215909 on OpenAlexafffund
Hsiu-Hsien Lin, Kai-Yang Lin, Chao-Te Li, Yao‐Huan Tseng, Homin Jiang, J.-H. Wang, Jen‐Chieh Cheng, Ue‐Li Pen, Ming‐Tang Chen, Pisin Chen, Yaocheng Chen, Tomotsugu Goto, T. Hashimoto, Yuh-Jing Hwang, Sun-Kun King, Derek Kubo, Chung-Yun Kuo, Adam J. Mills, J. W. Nam, Peter Oshiro, Chang-Shao Shen, Hsien‐Chun Tseng, Shih‐Hao Wang, Vigo Feng-Shun Wu, Geoffrey C. Bower, Shu-Hao Chang, Pai-An Chen, Ying‐Chih Chen, Yi-Kuan Chiang, Anatoli Fedynitch, Nina Gusinskaia, Simon C-C Ho, Tiger Yu-Yang Hsiao, Chin‐Ping Hu, Teddy Huang, José Miguel Jáuregui García, Seong Jin Kim, Decmend Fang-Jie Ling, Alvina Y L On, J. B. Peterson, Bjorn Jasper R. Raquel, Shih-Chieh Su, Yuri Uno, Cossas K-W Wu, Shotaro Yamasaki, Hong-Ming Zhu

Bibliographic record

VenuePublications of the Astronomical Society of the Pacific · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicRadio Astronomy Observations and Technology
Canadian institutionsUniversity of TorontoPerimeter InstituteCanadian Institute for Advanced ResearchCanadian Institute for Theoretical Astrophysics
FundersNatural Sciences and Engineering Research Council of CanadaNational Natural Science Foundation of ChinaCanadian Institute for Advanced ResearchAlexander von Humboldt-Stiftung
KeywordsAstronomyRadio telescopeTelescopePhysicsAstrophysics

Abstract

fetched live from OpenAlex

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.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.021
Threshold uncertainty score0.041

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0010.001
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0050.002

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.016
GPT teacher head0.214
Teacher spread0.198 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designBench or experimental
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations56
Published2022
Admission routes2
Has abstractyes

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