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Record W4361212630 · doi:10.3847/2041-8213/acbcd1

GRB 221009A: Discovery of an Exceptionally Rare Nearby and Energetic Gamma-Ray Burst

2023· article· en· W4361212630 on OpenAlexaff
Maia A. Williams, J. A. Kennea, S. Dichiara, Kohei Kobayashi, W. Iwakiri, A. P. Beardmore, P. A. Evans, Sebastian Heinz, A. Y. Lien, S. R. Oates, H. Negoro, S. B. Cenko, D. J. K. Buisson, D. H. Hartmann, Gaurava K. Jaisawal, N. P. M. Kuin, S. Lesage, K. L. Page, Tyler Parsotan, Dheeraj R. Pasham, B. Sbarufatti, M. H. Siegel, Satoshi Sugita, George Younes, E. Ambrosi, Zaven Arzoumanian, M. G. Bernardini, S. Campana, M. Capalbi, R. Caputo, A. D’Aì, P. D’Avanzo, V. D’Elia, M. de Pasquale, R. A. J. Eyles-Ferris, E. C. Ferrara, Keith C. Gendreau, J. D. Gropp, N. Kawai, N. J. Klingler, Sibasish Laha, A. Melandri, T. Mihara, M. J. Moss, P. T. O’Brien, J. P. Osborne, D. M. Palmer, M. Perri, Motoko Serino, Э. Сонбас, M. Stamatikos, R. L. C. Starling, G. Tagliaferri, A. Tohuvavohu, Silvia Zane, H. Ziaeepour

Bibliographic record

VenueThe Astrophysical Journal Letters · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsUniversity of Toronto
FundersJapan Aerospace Exploration AgencyMinistero dell’Istruzione, dell’Università e della RicercaScience and Technology Facilities CouncilUK Space AgencyUniversity of LeicesterPennsylvania State UniversityGoddard Space Flight CenterRIKENUniversity of PennsylvaniaNational Aeronautics and Space AdministrationOak Ridge Associated UniversitiesNational Science Foundation
KeywordsGamma-ray burstAstrophysicsPhysicsAstronomy

Abstract

fetched live from OpenAlex

Abstract We report the discovery of the unusually bright long-duration gamma-ray burst (GRB), GRB 221009A, as observed by the Neil Gehrels Swift Observatory (Swift), Monitor of All-sky X-ray Image, and Neutron Star Interior Composition Explorer Mission. This energetic GRB was located relatively nearby ( z = 0.151), allowing for sustained observations of the afterglow. The large X-ray luminosity and low Galactic latitude ( b = 4.°3) make GRB 221009A a powerful probe of dust in the Milky Way. Using echo tomography, we map the line-of-sight dust distribution and find evidence for significant column densities at large distances (≳10 kpc). We present analysis of the light curves and spectra at X-ray and UV–optical wavelengths, and find that the X-ray afterglow of GRB 221009A is more than an order of magnitude brighter at T 0 + 4.5 ks than that from any previous GRB observed by Swift. In its rest frame, GRB 221009A is at the high end of the afterglow luminosity distribution, but not uniquely so. In a simulation of randomly generated bursts, only 1 in 10 4 long GRBs were as energetic as GRB 221009A; such a large E γ ,iso implies a narrow jet structure, but the afterglow light curve is inconsistent with simple top-hat jet models. Using the sample of Swift GRBs with redshifts, we estimate that GRBs as energetic and nearby as GRB 221009A occur at a rate of ≲1 per 1000 yr—making this a truly remarkable opportunity unlikely to be repeated in our lifetime.

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: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.961
Threshold uncertainty score0.554

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 integrity0.0000.000
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 head0.009
GPT teacher head0.220
Teacher spread0.211 · 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 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

Citations111
Published2023
Admission routes1
Has abstractyes

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