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Record W4285220586 · doi:10.1093/mnras/stac1192

SN 2020acat: an energetic fast rising Type IIb supernova

2022· article· en· W4285220586 on OpenAlexafffund
K. Medler, P. A. Mazzali, Jacob Teffs, C. Ashall, J. P. Anderson, S. Benetti, K. Azalee Bostroem, J. Burke, P. Charalampopoulos, N. Elias–Rosa, M. Ergon, L. Galbany, M. Gromadzki, D. Hiramatsu, D. A. Howell, C. Inserra, Peter Lundqvist, C. McCully, T. E. Müller-Bravo, Megan Newsome, M. Nicholl, E. Paraskeva, A. Pastorello, C. Pellegrino, P. J. Pessi, A. Reguitti, T. Reynolds, R. Roy, G. Terreran, L. Tomasella, D. R. Young

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsCanadian Institute for Advanced Research
FundersH2020 European Research CouncilEuropean Social FundAgencia Estatal de InvestigaciónStockholms UniversitetScience and Technology Facilities CouncilAarhus UniversitetTurun YliopistoEuropean CommissionMinisterio de Ciencia e InnovaciónNuclear Safety and Security CommissionHáskóli ÍslandsNational Science FoundationLiverpool John Moores UniversityMinistero dell’Istruzione, dell’Università e della RicercaCouncil for Higher EducationAgencia Nacional de Investigación y DesarrolloFederación Española de Enfermedades RarasIsrael Science FoundationCanadian Institute for Advanced ResearchSuomalainen TiedeakatemiaAlbert Ellis InstituteUnited States-Israel Binational Science FoundationVetenskapsrådetConsejo Superior de Investigaciones CientíficasBonfils-Stanton FoundationVillum FondenNational Aeronautics and Space AdministrationAlan Turing InstituteUniversitetet i OsloChina Postdoctoral Science Foundation
KeywordsPhysicsSupernovaAstrophysicsAstronomyType (biology)Type II supernova

Abstract

fetched live from OpenAlex

ABSTRACT The ultraviolet (UV) and near-infrared (NIR) photometric and optical spectroscopic observations of SN 2020acat covering ∼250 d after explosion are presented here. Using the fast rising photometric observations, spanning from the UV to NIR wavelengths, a pseudo-bolometric light curve was constructed and compared to several other well-observed Type IIb supernovae (SNe IIb). SN 2020acat displayed a very short rise time reaching a peak luminosity of $\mathrm{{\rm Log}_{10}}(L) = 42.49 \pm 0.17 \, \mathrm{erg \, s^{-1}}$ in only ∼14.6 ± 0.3 d. From modelling of the pseudo-bolometric light curve, we estimated a total mass of 56Ni synthesized by SN 2020acat of MNi = 0.13 ± 0.03 M⊙, with an ejecta mass of Mej = 2.3 ± 0.4 M⊙ and a kinetic energy of Ek = 1.2 ± 0.3 × 1051 erg. The optical spectra of SN 2020acat display hydrogen signatures well into the transitional period (≳ 100 d), between the photospheric and the nebular phases. The spectra also display a strong feature around 4900 Å that cannot be solely accounted for by the presence of the Fe ii 5018 line. We suggest that the Fe ii feature was augmented by He i 5016 and possibly by the presence of N ii 5005. From both photometric and spectroscopic analysis, we inferred that the progenitor of SN 2020acat was an intermediate-mass compact star with an MZAMS of 15–20 M⊙.

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: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.008

Distilled classifier scores by category (both heads)

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)0.0010.000

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 head0.010
GPT teacher head0.213
Teacher spread0.203 · 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

Citations19
Published2022
Admission routes2
Has abstractyes

Explore more

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