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Record W2178172949 · doi:10.1126/science.aac7400

An extremely bright gamma-ray pulsar in the Large Magellanic Cloud

2015· article· en· W2178172949 on OpenAlexfundno aff
M. Ackermann, A. Albert, L. Baldini, J. Ballet, G. Barbiellini, C. Barbieri, D. Bastieri, R. Bellazzini, E. Bissaldi, R. Bonino, E. Bottacini, T. J. Brandt, J. Bregeon, P. Bruel, R. Buehler, G. A. Caliandro, R. A. Cameron, P. A. Caraveo, C. Cecchi, E. Charles, A. Chekhtman, C. C. Cheung, J. Chiang, G. Chiaro, S. Ciprini, J. Cohen-Tanugi, A. Cuoco, S. Cutini, F. D’Ammando, F. de Palma, S. W. Digel, L. Di Venere, P. S. Drell, C. Favuzzi, S. Fegan, E. C. Ferrara, A. Franckowiak, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Giglietto, F. Giordano, G. Godfrey, I. A. Grenier, M.-H. Grondin, J. E. Grove, L. Guillemot, S. Guiriec, Katsuro Hagiwara, A. K. Harding, E. Hays, John W. Hewitt, A. B. Hill, D. Horan, T. J. Johnson, J. Knödlseder, M. Kuss, S. Larsson, L. Latronico, M. Lemoine‐Goumard, J. Li, Liang Li, F. Longo, F. Loparco, M. N. Lovellette, P. Lubrano, S. Maldera, Alberto Manfreda, F. E. Marshall, Pierrick Martin, M. Mayer, M. N. Mazziotta, P. F. Michelson, N. Mirabal, Tsunefumi Mizuno, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, G. Naletto, E. Nuss, T. Ohsugi, M. Orienti, D. Paneque, M. Pesce-Rollins, F. Piron, G. Pivato, T. A. Porter, S. Rainò, R. Rando, M. Razzano, A. Reimer, O. Reimer, T. Reposeur, R. W. Romani, P. M. Saz Parkinson, A. Schulz, C. Sgró, E. J. Siskind, D. A. Smith, F. Spada, G. Spandre, P. Spinelli, D. J. Suson, H. Takahashi, J. B. Thayer, D. J. Thompson, L. Tibaldo, D. F. Torres, Y. Uchiyama, G. Vianello, K. S. Wood, M. Wood, L. Zampieri

Bibliographic record

VenueScience · 2015
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersIstituto Nazionale di Fisica NucleareCommissariat à l'Énergie Atomique et aux Énergies AlternativesAlberta InnovatesCentre National de la Recherche ScientifiqueInstitut National de Physique Nucléaire et de Physique des ParticulesVetenskapsrådetAgenzia Spaziale ItalianaScience and Technology Facilities CouncilMinistero dell’Istruzione, dell’Università e della RicercaCanada Research ChairsNational Aeronautics and Space AdministrationMinistry of Education, Culture, Sports, Science and TechnologyUniversity of AlbertaCMC MicrosystemsJapan Aerospace Exploration AgencyU.S. Department of Energy
KeywordsPhysicsPulsarAstrophysicsNeutron starAstronomyMilky WayLarge Magellanic CloudX-ray pulsarGalaxyGamma-ray astronomyBinary pulsarMillisecond pulsarSmall Magellanic CloudGamma rayCrab Pulsar

Abstract

fetched live from OpenAlex

Pulsars are rapidly spinning, highly magnetized neutron stars, created in the gravitational collapse of massive stars. We report the detection of pulsed giga-electron volt gamma rays from the young pulsar PSR J0540-6919 in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. This is the first gamma-ray pulsar detected in another galaxy. It has the most luminous pulsed gamma-ray emission yet observed, exceeding the Crab pulsar's by a factor of 20. PSR J0540-6919 presents an extreme test case for understanding the structure and evolution of neutron star magnetospheres.

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.002
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 communication0.0000.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.018
GPT teacher head0.266
Teacher spread0.247 · 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".

Quick stats

Citations50
Published2015
Admission routes1
Has abstractyes

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