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Record W4414818153 · doi:10.1093/mnras/staf1943

LOFAR constraints on the repetition and environments of CHIME FRBs

2025· article· en· W4414818153 on OpenAlexafffund
Pragya Chawla, A. Gopinath, Ninisha Manaswini, C. Bassa, J. W. T. Hessels, V. I. Kondratiev, Daniele Michilli, Ziggy Pleunis

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2025
Typearticle
Languageen
FieldEngineering
TopicAntenna Design and Optimization
Canadian institutionsMcGill University
FundersInstitut national des sciences de l'UniversScience and Technology Facilities CouncilObservatoire de Paris, Université de Recherche Paris Sciences et LettresMinisterium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-WestfalenH2020 European Research CouncilCentre National de la Recherche ScientifiqueUniversité d'OrléansMax-Planck-GesellschaftMinisterstwo Edukacji i NaukiCanada Excellence Research Chairs, Government of CanadaNederlandse Organisatie voor Wetenschappelijk OnderzoekBundesministerium für Bildung und ForschungUniversiteit van AmsterdamScience Foundation IrelandEuropean CommissionMcGill University
KeywordsLOFARRedshiftSpectral indexSupernovaFast radio burstRadio telescopeSupernova remnant

Abstract

fetched live from OpenAlex

ABSTRACT The behaviour of fast radio bursts (FRBs) at radio frequencies $< 400$ MHz is poorly understood, with only two sources detected below 300 MHz. We robustly characterize the 150-MHz activity of CHIME-detected FRB sources relative to their 600-MHz activity – using their non-detection in 473 h of archival observations from the LOFAR Tied-Array All-Sky Survey (LOTAAS), and in 252 h of LOFAR observations of 14 repeating FRB sources – the largest sub-300 MHz targeted FRB campaign to date. We search the LOTAAS data for repeat bursts from 33 CHIME/FRB repeaters, 10 candidate repeaters, and 430 apparent non-repeaters. Their non-detection yields a population-level statistical spectral index constraint of $\alpha _{s, 135\, \rm {MHz}/600\, \rm {MHz}}>-0.9$, indicating that FRB spectral indices are, on average, flatter than those of pulsars. From the targeted campaign, the prolific repeater FRB 20201124A shows $\alpha _s>0.55$, implying reduced low-frequency activity, unlike the typically negative $\alpha _ \rm {s}$ seen from FRBs at higher frequency bands. We explore free–free absorption in its circumburst environment as a cause of the non-detection at 150 MHz, and find that it is consistent with either a very young $\sim 10$ yr old supernova remnant; or a typical H ii region. Our simulations indicate that LOFAR2.0 can detect 0.3–9 FRBs per week, with up to 4 FRBs originating from redshifts $1< z< 3$. Such detections will provide robust constraints on cosmological parameters due to their clean environments. Our results thus inform future low-frequency FRB searches through the limits we place on repetition rates and show how even non-detections can place meaningful constraints on FRB circumburst environments.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.091
Threshold uncertainty score0.197

Codex and Gemma teacher scores by category

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

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 head0.004
GPT teacher head0.166
Teacher spread0.162 · 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 teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
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

Citations0
Published2025
Admission routes2
Has abstractyes

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