MétaCan
Menu
Back to cohort
Record W2955601320 · doi:10.1093/mnras/stz1811

The case for a high-redshift origin of GRB 100205A

2019· article· en· W2955601320 on OpenAlexfundno aff
A A Chrimes, A. J. Levan, E. R. Stanway, E. Berger, J. S. Bloom, S. B. Cenko, B. E. Cobb, Antonino Cucchiara, A. S. Fruchter, B. P. Gompertz, J. Hjorth, P. Jakobsson, J. Lyman, P. T. O’Brien, D. A. Perley, N. R. Tanvir, P. J. Wheatley, K. Wiersema

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersPlanetary Science DivisionScience and Technology Facilities CouncilScience Mission DirectorateSmithsonian Astrophysical ObservatoryUniversity of EdinburghMax-Planck-Institut für AstronomieComisión Nacional de Investigación Científica y TecnológicaNational Aeronautics and Space AdministrationEuropean Society of AnaesthesiologyEötvös Loránd TudományegyetemConsejo Nacional de Innovación, Ciencia y TecnologíaMinisterio de Ciencia, Tecnología e Innovación ProductivaQueen's UniversityMinisterio de Economía y CompetitividadUniversity of LeicesterKorea Astronomy and Space Science InstituteSpace Telescope Science InstituteUniversity of Hawai'iNational Central UniversityQueen's University BelfastGordon and Betty Moore FoundationLos Alamos National LaboratoryJohns Hopkins UniversityDurham UniversitySmithsonian InstitutionUniversity of MarylandMinistério da Ciência, Tecnologia e InovaçãoNational Science Foundation
KeywordsPhysicsGamma-ray burstRedshiftAstrophysicsAstronomyGalaxy

Abstract

fetched live from OpenAlex

Abstract The number of long gamma-ray bursts (GRBs) known to have occurred in the distant Universe (z > 5) is small (∼15); however, these events provide a powerful way of probing star formation at the onset of galaxy evolution. In this paper, we present the case for GRB 100205A being a largely overlooked high-redshift event. While initially noted as a high-z candidate, this event and its host galaxy have not been explored in detail. By combining optical and near-infrared Gemini afterglow imaging (at t < 1.3 d since burst) with deep late-time limits on host emission from the Hubble Space Telescope, we show that the most likely scenario is that GRB 100205A arose in the range 4 < z < 8. GRB 100205A is an example of a burst whose afterglow, even at ∼1 h post burst, could only be identified by 8-m class IR observations, and suggests that such observations of all optically dark bursts may be necessary to significantly enhance the number of high-redshift GRBs known.

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 categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.014

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 studies0.0010.001
Scholarly communication0.0020.001
Open science0.0000.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0040.001

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 head0.008
GPT teacher head0.217
Teacher spread0.208 · 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

Citations5
Published2019
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical SocietySame topicGamma-ray bursts and supernovaeFrench-language works237,207