MétaCan
Menu
Back to cohort
Record W2732898230 · doi:10.1093/mnras/stx2668

Supernovae 2016bdu and 2005gl, and their link with SN 2009ip-like transients: another piece of the puzzle

2017· article· en· W2732898230 on OpenAlexfundno aff
A. Pastorello, C. S. Kochanek, M. Fraser, Subo Dong, N. Elias–Rosa, A. V. Filippenko, S. Benetti, E. Cappellaro, L. Tomasella, A. J. Drake, J. Harmanen, T. Reynolds, B. J. Shappee, S. J. Smartt, K. C. Chambers, M. E. Huber, K. Smith, K. Z. Stanek, E. Christensen, L. Denneau, S. G. Djorgovski, H. Flewelling, C. Gall, A. Gal‐Yam, S. Geier, A. Heinze, T. W. S. Holoien, J. Isern, T. Kangas, E. Kankare, R. A. Koff, J. M. Llapasset, T. Lowe, P. Lundqvist, E. A. Magnier, S. Mattila, A. Morales-Garoffolo, R. L. Mutel, J. Nicolas, P. Ochner, E. O. Ofek, E. Prosperi, A. Rest, Y. Sano, B. Stalder, M. Stritzinger, F. Taddia, G. Terreran, J. Tonry, R. J. Wainscoat, C. Waters, H. Weiland, M. Willman, D. R. Young, WeiKang Zheng

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersPlanetary Science DivisionScience and Technology Facilities CouncilSmithsonian Astrophysical ObservatoryJet Propulsion LaboratoryInstituto de Astrofísica de CanariasMax-Planck-Institut für AstronomieEötvös Loránd TudományegyetemEmil Aaltosen SäätiöSuomen KulttuurirahastoChinese Academy of SciencesSmithsonian InstitutionU.S. Department of EnergyNational Natural Science Foundation of ChinaLiverpool John Moores UniversityNational Science FoundationScience Foundation IrelandFondo Nacional de Desarrollo Científico y TecnológicoQueen's UniversitySuomalainen TiedeakatemiaSeventh Framework ProgrammeEuropean Research CouncilGordon and Betty Moore FoundationQueen's University BelfastSpace Telescope Science InstituteCenter for Cosmology and Astroparticle Physics, Ohio State UniversityVillum FondenMinistero dell’Istruzione, dell’Università e della RicercaJohns Hopkins UniversityKey Laboratory of Particle Astrophysics, Institute of High Energy PhysicsIsrael Science FoundationChinese Academy of Sciences South America Center for AstronomyAspen Center for PhysicsIsraeli Centers for Research ExcellenceAdolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California BerkeleyOhio State UniversityScience Mission DirectorateU.S. Department of EducationEuropean CommissionCalifornia Institute of TechnologyPlanning and Budgeting Committee of the Council for Higher Education of IsraelNational Aeronautics and Space AdministrationDurham University
KeywordsPhysicsAstrophysicsSupernovaBalmer seriesLuminous blue variableSpectral linePair-instability supernovaEvent (particle physics)AstronomyEmission spectrumEjecta

Abstract

fetched live from OpenAlex

Supernova (SN) 2016bdu is an unusual transient resembling SN 2009ip. SN 2009ip-like events are characterized by a long-lasting phase of erratic variability that ends with two luminous outbursts a few weeks apart. The second outburst is significantly more luminous (about 3 mag) than the first. In the case of SN 2016bdu, the first outburst (Event A) reached an absolute magnitude M_r ≈ −15.3 mag, while the second one (Event B) occurred over one month later and reached M_r ≈ −18 mag. By inspecting archival data, a faint source at the position of SN 2016bdu is several times in the past few years. We interpret these detections as signatures of a phase of erratic variability, similar to that experienced by SN 2009ip between 2008 and mid-2012, and resembling the currently observed variability of the luminous blue variable SN 2000ch in NGC 3432. Spectroscopic monitoring of SN 2016bdu during the second peak initially shows features typical of an SN IIn. One month after the Event B maximum, the spectra develop broad Balmer lines with P Cygni profiles and broad metal features. At these late phases, the spectra resemble those of a typical Type II SN. All members of this SN 2009ip-like group are remarkably similar to the Type IIn SN 2005gl. For this object, the claim of a terminal SN explosion is supported by the disappearance of the progenitor star. While the similarity with SN 2005gl supports a genuine SN explosion scenario for SN 2009ip-like events, the unequivocal detection of nucleosynthesized elements in their nebular spectra is still missing.

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)0.001
metaresearch head score (Gemma)0.004
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 score0.005
Threshold uncertainty score0.014

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.004
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.002
Science and technology studies0.0010.002
Scholarly communication0.0030.003
Open science0.0010.002
Research integrity0.0050.003
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 head0.193
Teacher spread0.185 · 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

Citations77
Published2017
Admission routes1
Has abstractyes

Explore more

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