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Record W3082886691 · doi:10.3847/2041-8213/abbc02

Discovery of a Gamma-Ray Black Widow Pulsar by GPU-accelerated Einstein@Home

2020· article· en· W3082886691 on OpenAlexafffund
L. Nieder, C. J. Clark, D. Kandel, Roger W. Romani, C. Bassa, B. Allen, Abbarapu Ashok, I. Cognard, H. Fehrmann, P. C. C. Freire, R. Karuppusamy, Di Li, B. Machenschalk, Zhichen Pan, M. A. Papa, S. M. Ransom, Paul S. Ray, Jayanta Roy, Pei Wang, Jason Wu, C. Aulbert, E D Barr, Banafsheh Beheshtipour, O. Behnke, Bhaswati Bhattacharyya, R. P. Breton, F. Camilo, C. Choquet, V. S. Dhillon, E. C. Ferrara, L. Guillemot, J. W. T. Hessels, M. Kerr, S. Kwang, T. R. Marsh, M. B. Mickaliger, Ziggy Pleunis, H. J. Pletsch, M. S. Roberts, Siraprapa Sanpa-arsa, B. Steltner

Bibliographic record

VenueThe Astrophysical Journal Letters · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsMcGill University
FundersScience and Technology Facilities CouncilEuropean CommissionCanadian Institute for Advanced ResearchMax-Planck-GesellschaftNuclear Safety and Security CommissionDeutsche ForschungsgemeinschaftNational Aeronautics and Space AdministrationNational Science Foundation
KeywordsPulsarPhysicsMillisecond pulsarAstrophysicsFermi Gamma-ray Space TelescopeOrbital periodAstronomyBinary pulsarLight curvePulsar planetX-ray pulsarStars

Abstract

fetched live from OpenAlex

Abstract We report the discovery of 1.97 ms period gamma-ray pulsations from the 75 minute orbital-period binary pulsar now named PSR J1653−0158. The associated Fermi Large Area Telescope gamma-ray source 4FGL J1653.6−0158 has long been expected to harbor a binary millisecond pulsar. Despite the pulsar-like gamma-ray spectrum and candidate optical/X-ray associations—whose periodic brightness modulations suggested an orbit—no radio pulsations had been found in many searches. The pulsar was discovered by directly searching the gamma-ray data using the GPU-accelerated Einstein@Home distributed volunteer computing system. The multidimensional parameter space was bounded by positional and orbital constraints obtained from the optical counterpart. More sensitive analyses of archival and new radio data using knowledge of the pulsar timing solution yield very stringent upper limits on radio emission. Any radio emission is thus either exceptionally weak, or eclipsed for a large fraction of the time. The pulsar has one of the three lowest inferred surface magnetic-field strengths of any known pulsar with B surf ≈ 4 × 10 7 G. The resulting mass function, combined with models of the companion star’s optical light curve and spectra, suggests a pulsar mass ≳2 M ⊙ . The companion is lightweight with mass ∼0.01 M ⊙ , and the orbital period is the shortest known for any rotation-powered binary pulsar. This discovery demonstrates the Fermi Large Area Telescope's potential to discover extreme pulsars that would otherwise remain undetected.

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: Bench or experimental · Consensus signal: Bench or experimental
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.469
Threshold uncertainty score0.546

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 science0.0010.000
Research integrity0.0000.001
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 head0.014
GPT teacher head0.271
Teacher spread0.257 · 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 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

Citations69
Published2020
Admission routes2
Has abstractyes

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