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Record W4411483314 · doi:10.1051/0004-6361/202554988

Observational diversity of bright long-lived Type II supernovae

2025· article· en· W4411483314 on OpenAlexfundno aff
T. Nagao, H. Kuncarayakti, R. Cartier, S. Mattila, K. Maeda, J. Sollerman, P. J. Pessi, J. P. Anderson, C. Inserra, T. -W. Chen, Lucía Ferrari, M. Fraser, D. R. Young, M. Gromadzki, C. P. Gutiérrez, P. Lundqvist, G. Pignata, T.E Müller-Bravo, Fabio Ragosta, A. Reguitti, S. Moran, Maider González-Bañuelos, M. Kopsacheili, T. Petrushevska

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersJapan Society for the Promotion of ScienceUniversity of North Carolina at Chapel HillMax-Planck-Institut für AstronomieStockholms UniversitetUniversitetet i OsloMinistry of Education, IndiaMax-Planck-GesellschaftAgencia Estatal de InvestigaciónJavna Agencija za Raziskovalno Dejavnost RSHORIZON EUROPE Framework ProgrammeHáskóli ÍslandsNuclear Safety and Security CommissionQueen's UniversityMinisterio de Ciencia e InnovaciónAgencia Nacional de Investigación y DesarrolloGeneralitat de CatalunyaQueen's University BelfastSpace Telescope Science InstituteUniversity of PittsburghLos Alamos National LaboratoryCollege of Engineering, Michigan State UniversityAlfred P. Sloan FoundationUniversity of WashingtonPrinceton UniversityJohns Hopkins UniversityMichigan State UniversityScience and Technology Facilities CouncilTurun YliopistoAarhus UniversitetU.S. Naval ObservatoryU.S. Department of EnergyNew Mexico State UniversityFermilabNational Science FoundationAgència de Gestió d'Ajuts Universitaris i de RecercaMinistério da Ciência, Tecnologia e InovaçãoNational Aeronautics and Space Administration
KeywordsPhysicsAstrophysicsSupernovaObservational studyAstronomyType (biology)Diversity (politics)MedicineSociology

Abstract

fetched live from OpenAlex

Context. In various types of supernovae (SNe), strong interaction between the SN ejecta and circumstellar material (CSM) has been reported. This raises questions about their progenitors and mass-loss processes shortly before the explosion. Recently, the bright long-lived Type II SN 2021irp was proposed to be a standard Type II SN interacting with disk-like CSM. The observational properties suggest that the progenitor was a massive star (∼8−18 M⊙) in a binary system and underwent a mass-ejection process due to the binary interaction just before the explosion. Similar scenarios, i.e., a Type II SN interacting with a CSM disk, have also been invoked to explain some Type IIn SNe. Aims. Here, we study the diversity of the observational properties of bright long-lived Type II (21irp-like) SNe. We analyze the diversity of their CSM properties, in order to understand their progenitors and mass-loss mechanisms and their relations with the other types of interacting SNe. Methods. We performed photometry, spectroscopy, and/or polarimetry for four 21irp-like SNe. Based on these observations as well as published data of SN 2021irp itself and well-observed bright and long-lived type II SNe including SNe 2010jl, 2015da, and 2017hcc, we discuss their CSM characteristics. Results. This sample of SNe shows luminous and long-lived photometric evolution, with some variations in the photometric evolution (from ∼−17 to ∼−20 absolute mag in the r/o band even at ∼200 days after the explosion). They show photospheric spectra characterized mainly by Balmer lines for several hundreds of days, with some variations in the shapes of the lines. They show high polarization with slight variations in the polarization degrees (∼1−3% at the brightness peak) with rapid declines with time (from ∼3−6% before the peak to ∼1% at ∼200 days after the peak). The general observational properties are consistent with the disk-CSM-interaction scenario, i.e., typical Type II SNe interacting with disk-like CSM. At the same time, the variation in the observational properties suggest diversity in the CSM mass and the opening angle of the CSM disk. These variations in the CSM properties are likely to be be related to the binary parameters of the progenitor systems and/or the properties of the progenitor and companion stars.

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)0.002
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 score0.002
Threshold uncertainty score0.005

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
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 head0.019
GPT teacher head0.228
Teacher spread0.209 · 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

Citations2
Published2025
Admission routes1
Has abstractyes

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