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Record W2993908089 · doi:10.1093/mnras/stz3390

Nebular spectra of 111 Type Ia supernovae disfavour single-degenerate progenitors

2019· article· en· W2993908089 on OpenAlexfundno aff
M. A. Tucker, B. J. Shappee, P. Vallely, K. Z. Stanek, J. L. Prieto, J. Botyánszki, C. S. Kochanek, J. P. Anderson, J. S. Brown, L. Galbany, T. W. S. Holoien, E. Y. Hsiao, Sahana Kumar, H. Kuncarayakti, N. Morrell, M. M. Phillips, M. Stritzinger, Todd A. Thompson

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersPlanetary Science DivisionScience Mission DirectorateLeibniz-Institut für Astrophysik PotsdamEötvös Loránd TudományegyetemMinisterio de Ciencia, Tecnología e Innovación ProductivaDanmarks Frie ForskningsfondGordon and Betty Moore FoundationQueen's University BelfastMax-Planck-Institut für AstronomieUniversity of EdinburghSpace Telescope Science InstituteSmithsonian Astrophysical ObservatoryArizona Board of RegentsRadcliffe Institute for Advanced Study, Harvard UniversityNational Central UniversityVillum FondenLos Alamos National LaboratoryEuropean Space AgencyJohns Hopkins UniversityFondo Nacional de Desarrollo Científico y TecnológicoHarvard UniversityQueen's UniversityOhio State UniversityLeibniz-GemeinschaftUniversity of Notre DameUniversity of ArizonaEuropean School of OncologyNational Science FoundationUniversity of MinnesotaCalifornia Institute of TechnologyMinisterio de Economía, Fomento y Turismo, ChileSmithsonian InstitutionU.S. Department of EnergyMinistério da Ciência, Tecnologia e InovaçãoComisión Nacional de Investigación Científica y TecnológicaNational Aeronautics and Space AdministrationIstituto Nazionale di AstrofisicaDurham University
KeywordsPhysicsSupernovaAstrophysicsChandrasekhar limitWhite dwarfDegenerate energy levelsSpectral lineBrightnessLimit (mathematics)Type (biology)AstronomyStarsQuantum mechanics

Abstract

fetched live from OpenAlex

ABSTRACT We place statistical constraints on Type Ia supernova (SN Ia) progenitors using 227 nebular-phase spectra of 111 SNe Ia. We find no evidence of stripped companion emission in any of the nebular-phase spectra. Upper limits are placed on the amount of mass that could go undetected in each spectrum using recent hydrodynamic simulations. With these null detections, we place an observational 3σ upper limit on the fraction of SNe Ia that are produced through the classical H-rich non-degenerate companion scenario of $\lt 5.5 {{\ \rm per\ cent}}$. Additionally, we set a tentative 3σ upper limit otan He star progenitor scenarios of $\lt 6.4 {{\ \rm per\ cent}}$, although further theoretical modelling is required. These limits refer to our most representative sample including normal, 91bg-like, 91T-like, and ‘super-Chandrasekhar’ SNe Ia but excluding SNe Iax and SNe Ia-CSM. As part of our analysis, we also derive a Nebular Phase Phillips Relation, which approximates the brightness of an SN Ia from 150 to 500 d after maximum using the peak magnitude and decline rate parameter Δm15(B).

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 score0.002
Threshold uncertainty score0.005

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
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 head0.009
GPT teacher head0.204
Teacher spread0.196 · 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

Citations63
Published2019
Admission routes1
Has abstractyes

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