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Strongly polarised radio pulses from a new white-dwarf-hosting long-period transient

2025· article· en· W7116045293 on OpenAlexfundno aff

Bibliographic record

VenueSpringer Link (Chiba Institute of Technology) · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersPlanetary Science DivisionScience and Technology Facilities CouncilObservatoire de Paris, Université de Recherche Paris Sciences et LettresScience Mission DirectorateSmithsonian Astrophysical ObservatoryMax-Planck-Institut für AstronomieMinisterium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-WestfalenDurham UniversityIstituto Nazionale di AstrofisicaCentre National de la Recherche ScientifiqueMax-Planck-GesellschaftNederlandse Organisatie voor Wetenschappelijk OnderzoekQueen's UniversityBundesministerium für Bildung und ForschungNational Science FoundationScience Foundation IrelandUK Research and InnovationSpace Telescope Science InstituteNational Central UniversityQueen's University BelfastGordon and Betty Moore FoundationEötvös Loránd TudományegyetemEuropean CommissionLos Alamos National LaboratoryJohns Hopkins UniversityUniversité d'OrléansNational Aeronautics and Space AdministrationSmithsonian Institution
KeywordsWhite dwarfPulse (music)Duty cycleTransient (computer programming)SkyLOFARMagnitude (astronomy)Flare

Abstract

fetched live from OpenAlex

Long-period transients (LPTs) are a new and enigmatic class of objects that produce bright pulsations in the radio, with periods far exceeding those seen in rotationally powered pulsars. The proposed progenitors for LPTs are contested, with white dwarfs or magnetars being likely candidates. Here, we present the discovery of ILT J163430+445010, a new LPT detected in a blind search for Stokes V transients in the LOFAR Two-Metre Sky Survey. Unusual for LPTs, J1634+44 shows pulses that are 100% circularly polarised, as well as pulses that are 100% linearly polarised, with the polarisation state changing from pulse to pulse. We detect 19 pulses in total, each with a total polarisation fraction of ∼100% and a pulse duration of at most 10 s. The pulses show a periodicity at 841.24808±0.00015 s, implying a low duty cycle of 0.012. J1634+44 has a marginally detected counterpart in the ultraviolet GALEX MIS survey and the ultraviolet/optical UNIONS survey, suggesting that it contains a white dwarf with an effective temperature between 15 000 K and 33 000 K. We do not detect J1634+44 with a deep J-band exposure with UKIRT at a 3σ AB magnitude limit of 24.7, ruling out a main-sequence star or ultracool dwarf with a spectral type earlier than M7. The pulses from J1634+44 follow a particular pattern, with two pulses being produced every five periods after a waiting time of two or three periods. This pattern could be a result of spin-orbit coupling in a binary system with a 5:2 or 5:3 resonance, where a companion induces beamed radio emission on the white dwarf. The companion is most likely an ultracool dwarf or another white dwarf, making J1634+44 unique among the currently known sample of LPTs.

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)0.000
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: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.001
Threshold uncertainty score0.004

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.011
GPT teacher head0.281
Teacher spread0.270 · 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 designObservational
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".

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Citations0
Published2025
Admission routes1
Has abstractyes

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