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Record W3160117467 · doi:10.1093/mnras/staa2763

SN 2017ivv: two years of evolution of a transitional Type II supernova

2020· article· en· W3160117467 on OpenAlexafffund
C. P. Gutiérrez, A. Pastorello, Anders Jerkstrand, L. Galbany, M. Sullivan, J. P. Anderson, S. Taubenberger, H. Kuncarayakti, S. González–Gaitán, P. Wiseman, C. Inserra, M. Fraser, K. Maguire, S. J. Smartt, T. E. Müller-Bravo, S. Benetti, D. Bersier, S. Bose, K. Azalee Bostroem, J. Burke, Ping Chen, M. Della Valle, Subo Dong, A. Gal‐Yam, M. Gromadzki, D. Hiramatsu, T. W. S. Holoien, G. Hosseinzadeh, D. A. Howell, E. Kankare, C. S. Kochanek, C. McCully, M. Nicholl, G. Pignata, J. L. Prieto, B. J. Shappee, K. Taggart, L. Tomasella, S. Valenti, D. R. Young

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsCanadian Institute for Advanced Research
FundersH2020 European Research CouncilScience and Technology Facilities CouncilMax-Planck-GesellschaftVillum FondenCenter for Cosmology and Astroparticle Physics, Ohio State UniversityNational Science FoundationScience Foundation IrelandLiverpool John Moores UniversityChinese Academy of SciencesDeutsche ForschungsgemeinschaftGordon and Betty Moore FoundationQueen's University BelfastCalifornia Institute of TechnologyEuropean CommissionLeibniz-GemeinschaftJet Propulsion LaboratoryChinese Academy of Sciences South America Center for AstronomyW. M. Keck FoundationSpace Telescope Science InstituteQueen's UniversityOhio State UniversityRoyal Astronomical SocietyNuclear Safety and Security CommissionComisión Nacional de Investigación Científica y TecnológicaNational Aeronautics and Space Administration
KeywordsPhysicsSupernovaAstrophysicsLight curveGalaxySpectral lineRadioactive decayType (biology)Phase (matter)AstronomyAtomic physics

Abstract

fetched live from OpenAlex

ABSTRACT We present the photometric and spectroscopic evolution of the Type II supernova (SN II) SN 2017ivv (also known as ASASSN-17qp). Located in an extremely faint galaxy (Mr = −10.3 mag), SN 2017ivv shows an unprecedented evolution during the 2 yr of observations. At early times, the light curve shows a fast rise (∼6−8 d) to a peak of ${\it M}^{\rm max}_{g}= -17.84$ mag, followed by a very rapid decline of 7.94 ± 0.48 mag per 100 d in the V band. The extensive photometric coverage at late phases shows that the radioactive tail has two slopes, one steeper than that expected from the decay of 56Co (between 100 and 350 d), and another slower (after 450 d), probably produced by an additional energy source. From the bolometric light curve, we estimated that the amount of ejected 56Ni is ∼0.059 ± 0.003 M⊙. The nebular spectra of SN 2017ivv show a remarkable transformation that allows the evolution to be split into three phases: (1) Hα strong phase (<200 d); (2) Hα weak phase (between 200 and 350 d); and (3) Hα broad phase (>500 d). We find that the nebular analysis favours a binary progenitor and an asymmetric explosion. Finally, comparing the nebular spectra of SN 2017ivv to models suggests a progenitor with a zero-age main-sequence mass of 15–17 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)0.001
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 score0.005
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.001
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 head0.011
GPT teacher head0.210
Teacher spread0.199 · 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

Citations22
Published2020
Admission routes2
Has abstractyes

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