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A nearby long gamma-ray burst from a merger of compact objects

2022· article· en· 269 citations· W4311421419 on OpenAlex· 10.1038/s41586-022-05327-3

Why is this work in the frame?

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

Canadian affiliationAn author listed a Canadian institution. This is the only route the usual frame has.
Canadian funderA Canadian agency funded it. The work may carry no Canadian affiliation at all.

Full frame distilled prediction

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.

Candidate categories
Insufficient payload (model declined to judge)
Consensus categories
none
Domain
Candidate signal: noneConsensus signal: none
Study design
Candidate signal: ObservationalConsensus signal: Observational
Genre
Candidate signal: EmpiricalConsensus signal: Empirical
Teacher disagreement score
0.183
Threshold uncertainty score
0.995
Validation status
machine_predicted_unvalidated · codex-gemma-dda1882f352a

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 integrity0.0000.002
Insufficient payload (model declined to judge)0.0060.000

Machine scores (provisional)

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

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.

Opus teacher head0.008
GPT teacher head0.236
Teacher spread
0.229 · how far apart the two teachers sit on this one work
Validation status
score_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Abstract

Abstract Gamma-ray bursts (GRBs) are flashes of high-energy radiation arising from energetic cosmic explosions. Bursts of long (greater than two seconds) duration are produced by the core-collapse of massive stars 1 , and those of short (less than two seconds) duration by the merger of compact objects, such as two neutron stars 2 . A third class of events with hybrid high-energy properties was identified 3 , but never conclusively linked to a stellar progenitor. The lack of bright supernovae rules out typical core-collapse explosions 4–6 , but their distance scales prevent sensitive searches for direct signatures of a progenitor system. Only tentative evidence for a kilonova has been presented 7,8 . Here we report observations of the exceptionally bright GRB 211211A, which classify it as a hybrid event and constrain its distance scale to only 346 megaparsecs. Our measurements indicate that its lower-energy (from ultraviolet to near-infrared) counterpart is powered by a luminous (approximately 10 42 erg per second) kilonova possibly formed in the ejecta of a compact object merger.

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.

The record

Venue
Nature
Topic
Gamma-ray bursts and supernovae
Field
Physics and Astronomy
Canadian institutions
Perimeter Institute
Funders
Los Alamos National LaboratoryInstitute for Cosmic Ray Research, University of TokyoJapan Society for the Promotion of ScienceNational Nuclear Security AdministrationInstitut Périmètre de physique théoriqueMinistry of Education, Culture, Sports, Science and TechnologyInstituto de Astrofísica de AndalucíaUniversity of TokyoU.S. Department of EnergyEuropean CommissionNuclear Safety and Security CommissionAgencia Nacional de Investigación y DesarrolloDepartment of Science and Technology, Ministry of Science and Technology, IndiaUniversity of ToledoUniversity of LeicesterIndian Space Research OrganisationKorea Astronomy and Space Science InstituteSpace Telescope Science InstituteConsejo Superior de Investigaciones CientíficasMinistry of Colleges and UniversitiesGovernment of CanadaJunta de AndalucíaNational Science FoundationNorthern Arizona UniversityYale UniversityNational Aeronautics and Space Administration
Keywords
AstrophysicsPhysicsGamma-ray burstAstronomy
Has abstract in OpenAlex
yes