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Record W3112028838

[no title]

2019· article· en· W3112028838 on OpenAlexfundno aff
Hans van Haren, I. Ansseau, Paul Coppin, Pablo Correa, C. De Clercq, S. De Ridder, G. de Wasseige, D. Heereman, N. Iovine, M. Labare, J. Lünemann, G. Maggi, K. Meagher, T. Meures, A. O’Murchadha, E. Pinat, Christoph Raab, Giovanni Renzi, D. Ryckbosch, S. Toscano, W. Van Driessche, S. Vanheule, M. Vraeghe, B. Ding, J. Watchi

Bibliographic record

VenuePortsmouth Research Portal (University of Portsmouth) · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersNational Research, Development and Innovation OfficeInstitute for Global Prominent Research, Chiba UniversityInstitut National de Physique Nucléaire et de Physique des ParticulesLabex UnivEarthSDeutsches Elektronen-SynchrotronAgencia Estatal de InvestigaciónGovern de les Illes BalearsMarsden FundHelmholtz Alliance for Astroparticle PhysicsIstituto Nazionale di Fisica NucleareConseil Régional Provence-Alpes-Côte d'AzurRWTH Aachen UniversityJapan Society for the Promotion of ScienceVillum FondenInstitut Universitaire de FranceMinistry of Education, IndiaCollege of Engineering, Michigan State UniversityScottish Funding CouncilKnut och Alice Wallenbergs StiftelseIndustry CanadaCommissariat à l'Énergie Atomique et aux Énergies AlternativesConseil Régional d'AlsaceHungarian Scientific Research FundGeneralitat ValencianaFonds Wetenschappelijk OnderzoekFonds De La Recherche Scientifique - FNRSRussian Foundation for Basic ResearchDivision of Human Resource DevelopmentMinistero dello Sviluppo EconomicoDanmarks GrundforskningsfondScience and Technology Facilities CouncilSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungKavli FoundationAgence Nationale de la RechercheEuropean Regional Development FundICTP South American Institute for Fundamental ResearchCentre National de la Recherche ScientifiqueCouncil of Scientific and Industrial Research, IndiaRussian Science FoundationOffice of Polar ProgramsMichigan State UniversityEuropean CommissionLeverhulme TrustDeutsche ForschungsgemeinschaftNederlandse Organisatie voor Wetenschappelijk OnderzoekScience and Engineering Research BoardPolarforskningssekretariatetNational Natural Science Foundation of ChinaScottish Universities Physics AllianceNational Research Foundation of KoreaNemzeti Kutatási Fejlesztési és Innovációs HivatalNational Research FoundationWestern Canada Research GridNatural Sciences and Engineering Research Council of CanadaMinisterio de Economía y CompetitividadBundesministerium für Bildung und ForschungInstitut des Origines de LyonCanadian Institute for Advanced ResearchAutoritatea Natională pentru Cercetare StiintificăVetenskapsrådetU.S. Department of EnergyUniversity of Wisconsin-MadisonChiba UniversityRoyal SocietyBelgian Federal Science Policy OfficeNational Science FoundationCompute CanadaMarquette UniversityAbdus Salam International Centre for Theoretical Physics
KeywordsPhysicsLIGOGravitational waveNeutrinoAstrophysicsAstronomyNeutron starSupernovaGravitational-wave astronomyPulsarParticle physics
DOInot available

Abstract

fetched live from OpenAlex

Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.

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)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Other · Consensus signal: Other
Teacher disagreement score0.912
Threshold uncertainty score0.000

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0880.016

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 head0.021
GPT teacher head0.259
Teacher spread0.238 · 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.

Study designNot applicable
Domainnot available
GenreOther

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

Citations19
Published2019
Admission routes1
Has abstractyes

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