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Record W2161826059 · doi:10.1093/mnras/stv1097

The rise-time of Type II supernovae

2015· article· en· W2161826059 on OpenAlexaff
S. González–Gaitán, Nozomu Tominaga, Juan Molina, L. Galbany, F. Bufano, J. P. Anderson, C. P. Gutiérrez, F. Förster, G. Pignata, Melina C. Bersten, D. A. Howell, M. Sullivan, R. G. Carlberg, Thomas de Jaeger, M. Hamuy, П. В. Бакланов, С. И. Блинников

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2015
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsUniversity of Toronto
FundersU.S. Department of EnergyU.S. Naval ObservatoryMax-Planck-Institut für AstronomieMax-Planck-GesellschaftCentre National de la Recherche ScientifiqueChinese Academy of SciencesUniversity of PittsburghUniversity of CambridgeNew Mexico State UniversityUniversity of PortsmouthNational Aeronautics and Space AdministrationComisión Nacional de Investigación Científica y TecnológicaUniversität BaselLos Alamos National LaboratoryAlfred P. Sloan FoundationUniversity of WashingtonPrinceton UniversityJohns Hopkins UniversitySchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungOhio State UniversityRussian Science FoundationFermilabCase Western Reserve UniversityNational Science FoundationDrexel University
KeywordsPhysicsRed supergiantSupernovaAstrophysicsRADIUSSolar radiusLight curveWavelengthSkyShock (circulatory)AstronomySupergiantStarsOpticsCoronal mass ejectionPlasma

Abstract

fetched live from OpenAlex

We investigate the early-time light curves of a large sample of 223 Type II supernovae (SNe II) from the Sloan Digital Sky Survey and the Supernova Legacy Survey. Having a cadence of a few days and sufficient non-detections prior to explosion, we constrain risetimes, i.e. the durations from estimated first to maximum light, as a function of effective wavelength. At rest-frame g 0 band ( eff = 4722 ), we find a distribution of fast rise-times with median of (7.5 0.3) d. Comparing these durations with analytical shock models of Rabinak & Waxman and Nakar & Sari, and hydrodynamical models of Tominaga et al., which are mostly sensitive to progenitor radius at these epochs, we find a median characteristic radius of less than 400 solar radii. The inferred radii are on average much smaller than the radii obtained for observed red supergiants (RSG). Investigating the post-maximum slopes as a function of effective wavelength in the light of theoretical models, we find that massive hydrogen envelopes are still needed to explain the plateaus of SNe II. We therefore argue that the SN II rise-times we observe are either (a) the shock cooling resulting from the core collapse of RSG with small and dense envelopes, or (b) the delayed and prolonged shock breakout of the collapse of an RSG with an extended atmosphere or embedded within pre-SN circumstellar material.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation 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 score0.217
Threshold uncertainty score0.415

Codex and Gemma teacher scores by category

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 science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.012
GPT teacher head0.214
Teacher spread0.202 · 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 teacher head, 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

Citations148
Published2015
Admission routes1
Has abstractyes

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