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Record W2116228165 · doi:10.1051/0004-6361/201423387

GRB 120422A/SN 2012bz: Bridging the gap between low- and high-luminosity gamma-ray bursts

2014· article· en· W2116228165 on OpenAlexfundno aff
S. Schulze, D. Malesani, Antonino Cucchiara, N. R. Tanvir, T. Krühler, A. de Ugarte Postigo, G. Leloudas, J. Lyman, D. Bersier, K. Wiersema, D. A. Perley, P. Schady, J. Gorosabel, J. P. Anderson, A. J. Castro‐Tirado, S. B. Cenko, A. De, L. E. Ellerbroek, J. P. U. Fynbo, J. Greiner, J. Hjorth, Д. А. Канн, L. Kaper, S. Klose, A. J. Levan, S. Martín, P. T. O’Brien, K. L. Page, G. Pignata, Sarah Grace Rapaport, R. Sánchez-Ramírez, J. Sollerman, I. A. Smith, Martin Sparre, C. C. Thöne, D. Watson, D. Xu, F. E. Bauer, Matthew Bayliss, G. Björnsson, Michael Bremer, Z. Cano, S. Covino, V. D’Elia, D. A. Frail, S. Geier, P. Goldoni, O. E. Hartoog, P. Jakobsson, H. Korhonen, K. Y. Lee, B. Milvang‐Jensen, M. Nardini, A. Nicuesa Guelbenzu, Masamune Oguri, S. B. Pandey, G. Petitpas, A. Rossi, Andreas Sandberg, G. Tagliaferri, R. P. J. Tilanus, J. M. Winters, D. E. Wright, Eva Wuyts

Bibliographic record

VenueAstronomy and Astrophysics · 2014
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersFP7 People: Marie-Curie ActionsLawrence Berkeley National LaboratoryFondo de Innovación para la CompetitividadComisión Nacional de Investigación Científica y TecnológicaLeibniz-GemeinschaftMinisterio de Economía, Fomento y Turismo, ChileYork UniversityScience and Technology Facilities CouncilSmithsonian Astrophysical ObservatoryInstituto de Astrofísica de CanariasHáskóli ÍslandsW. M. Keck FoundationThüringer Ministerium für Bildung, Wissenschaft und KulturHebrew University of JerusalemUniversidad Andrés BelloAcademia SinicaNederlandse Organisatie voor Wetenschappelijk OnderzoekDeutsche ForschungsgemeinschaftEuropean CommissionBrookhaven National LaboratoryJames S. McDonnell FoundationCentre National de la Recherche ScientifiqueMax-Planck-GesellschaftUniversity of LeicesterCarnegie Mellon UniversityCollege of Engineering, Michigan State UniversityMinisterul Educaţiei NaţionaleUniversity of WashingtonAlfred P. Sloan FoundationPrinceton UniversityJohns Hopkins UniversityVanderbilt UniversityUniversity of ChicagoHarvard UniversityNational Research FoundationOhio State UniversityVetenskapsrådetYale UniversityU.S. Department of EnergySmithsonian InstitutionDanmarks GrundforskningsfondNational Aeronautics and Space AdministrationGordon and Betty Moore FoundationCalifornia Institute of TechnologyUniversity of ArizonaWeizmann Institute of ScienceAlexander von Humboldt-StiftungNew Mexico State UniversityUniversity of PortsmouthKenneth T. and Eileen L. Norris FoundationOffice of ScienceNational Science Foundation
KeywordsPhysicsAstrophysicsGamma-ray burstRedshiftGalaxySupernovaLuminositySpectral energy distributionStar formationAstronomy

Abstract

fetched live from OpenAlex

Context. At low redshift, a handful of gamma-ray bursts (GRBs) have been discovered with luminosities that are substantially lower (L iso < 10 48.5 erg s -1 ) than the average of more distant ones (L iso > 10 49.5 erg s -1 ). It has been suggested that the properties of several low-luminosity (low-L) GRBs are due to shock break-out, as opposed to the emission from ultrarelativistic jets. This has led to much debate about how the populations are connected. Aims. The burst at redshift z = 0.283 from 2012 April 22 is one of the very few examples of intermediate-L GRBs with a -ray luminosity of L iso 10 49.6-49.9 erg s -1 that have been detected up to now. With the robust detection of its accompanying supernova SN 2012bz, it has the potential to answer important questions on the origin of low-and high-L GRBs and the GRB-SN connection. Methods. We carried out a spectroscopy campaign using medium-and low-resolution spectrographs with 6-10-m class telescopes, which covered a time span of 37.3 days, and a multi-wavelength imaging campaign, which ranged from radio to X-ray energies over a duration of 270 days. Furthermore, we used a tuneable filter that is centred at H to map star-formation in the host and the surrounding galaxies. We used these data to extract and model the properties of different radiation components and fitted the spectral energy distribution to extract the properties of the host galaxy.

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 categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.434
Threshold uncertainty score1.000

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 studies0.0010.000
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 head0.204
Teacher spread0.195 · 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.

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

Citations131
Published2014
Admission routes1
Has abstractyes

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