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Record W4383472826 · doi:10.1038/s41586-023-06759-1

Heavy-element production in a compact object merger observed by JWST

2023· preprint· en· W4383472826 on OpenAlexafffund
A. J. Levan, B. P. Gompertz, O. S. Salafia, Mattia Bulla, Eric Burns, Kenta Hotokezaka, L. Izzo, Gavin P. Lamb, D. Malesani, S. R. Oates, M. E. Ravasio, Alicia Rouco Escorial, Benjamin Schneider, Nikhil Sarin, S. Schulze, N. R. Tanvir, K. Ackley, G. E. Anderson, Gabriel Brammer, L. Christensen, V. S. Dhillon, P. A. Evans, Michael Fausnaugh, Wen‐fai Fong, A. S. Fruchter, Chris L. Fryer, J. P. U. Fynbo, Nicola Gaspari, K. E. Heintz, J. Hjorth, J. A. Kennea, Mark Kennedy, T. Laskar, G. Leloudas, Ilya Mandel, A. Martín-Carrillo, Brian D. Metzger, M. Nicholl, Anya E. Nugent, J. T. Palmerio, G. Pugliese, Jillian Rastinejad, L. Rhodes, A. Rossi

Bibliographic record

VenueNature · 2023
Typepreprint
Languageen
FieldEngineering
TopicAdvanced X-ray and CT Imaging
Canadian institutionsUniversity of Toronto
FundersPlanetary Science DivisionJapan Society for the Promotion of ScienceScience Mission DirectorateSmithsonian Astrophysical ObservatoryJet Propulsion LaboratoryInstituto de Astrofísica de CanariasMax-Planck-Institut für AstronomieAgencia Nacional de Investigación y DesarrolloEötvös Loránd TudományegyetemUniversity of California, Los AngelesStockholms UniversitetUniversitetet i OsloMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesKorea Astronomy and Space Science InstituteSpace Telescope Science InstituteEuropean Southern ObservatoryCentre National d’Etudes SpatialesNational Aeronautics and Space AdministrationDanmarks GrundforskningsfondNational Research FoundationGordon and Betty Moore FoundationQueen's University BelfastQueen's UniversityNederlandse Organisatie voor Wetenschappelijk OnderzoekNordForskSmithsonian InstitutionVetenskapsrådetDurham UniversityNorthwestern UniversityNational Central UniversityVillum FondenLos Alamos National LaboratoryJohns Hopkins UniversityEuropean CommissionCalifornia Institute of TechnologyScience and Technology Facilities CouncilTurun YliopistoAarhus UniversitetUniversity of LeicesterUniversità degli Studi di FerraraHáskóli ÍslandsNuclear Safety and Security CommissionNational Science Foundation
KeywordsPhysicsKilonovaGamma-ray burstNeutron starAstrophysicsNucleosynthesisGravitational waveCompact starAstronomyr-processAccretion (finance)Black hole (networking)GalaxyStars

Abstract

fetched live from OpenAlex

Abstract The mergers of binary compact objects such as neutron stars and black holes are of central interest to several areas of astrophysics, including as the progenitors of gamma-ray bursts (GRBs) 1 , sources of high-frequency gravitational waves (GWs) 2 and likely production sites for heavy-element nucleosynthesis by means of rapid neutron capture (the r -process) 3 . Here we present observations of the exceptionally bright GRB 230307A. We show that GRB 230307A belongs to the class of long-duration GRBs associated with compact object mergers 4–6 and contains a kilonova similar to AT2017gfo, associated with the GW merger GW170817 (refs. 7–12 ). We obtained James Webb Space Telescope (JWST) mid-infrared imaging and spectroscopy 29 and 61 days after the burst. The spectroscopy shows an emission line at 2.15 microns, which we interpret as tellurium (atomic mass A = 130) and a very red source, emitting most of its light in the mid-infrared owing to the production of lanthanides. These observations demonstrate that nucleosynthesis in GRBs can create r -process elements across a broad atomic mass range and play a central role in heavy-element nucleosynthesis across the Universe.

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 score0.001
Threshold uncertainty score0.003

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0010.000
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 head0.022
GPT teacher head0.272
Teacher spread0.250 · 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

Citations212
Published2023
Admission routes2
Has abstractyes

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