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Record W1894385335 · doi:10.3847/0004-637x/819/1/35

RAPIDLY RISING TRANSIENTS IN THE SUPERNOVA—SUPERLUMINOUS SUPERNOVA GAP

2016· article· en· W1894385335 on OpenAlexafffund
I. Arcavi, William M. Wolf, D. A. Howell, Lars Bildsten, G. Leloudas, D. Hardin, S. Prajs, D. A. Perley, Gilad Svirski, A. Gal‐Yam, Boaz Katz, C. McCully, S. B. Cenko, C. Lidman, M. Sullivan, S. Valenti, P. Astier, C. Balland, R. G. Carlberg, Alex Conley, D. Fouchez, J. Guy, R. Pain, N. Palanque‐Delabrouille, Kathy Perrett, C. J. Pritchet, N. Regnault, V. Ruhlmann-Kleider

Bibliographic record

VenueThe Astrophysical Journal · 2016
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsUniversity of VictoriaDefence Research and Development CanadaUniversity of Toronto
FundersLawrence Berkeley National LaboratoryBrookhaven National LaboratoryScience and Technology Facilities CouncilIsrael Science FoundationPlanning and Budgeting Committee of the Council for Higher Education of IsraelComisión Nacional de Investigación Científica y TecnológicaNational Aeronautics and Space AdministrationDanmarks GrundforskningsfondYork UniversityOhio State UniversityNational Research FoundationCarnegie Mellon UniversityOffice of ScienceUniversity of WashingtonAlfred P. Sloan FoundationPrinceton UniversityJohns Hopkins UniversityCollege of Engineering, Michigan State UniversityHarvard UniversityNew Mexico State UniversityUniversity of PortsmouthYale UniversityVanderbilt UniversityJet Propulsion LaboratoryCalifornia Institute of TechnologyU.S. Department of EnergyW. M. Keck FoundationNational Science Foundation
KeywordsSupernovaPhysicsAstrophysicsMagnetarLight curveGamma-ray burstWhite dwarfAstronomySpectral lineStarsNeutron star

Abstract

fetched live from OpenAlex

ABSTRACT We present observations of four rapidly rising ( t rise ≈ 10 days) transients with peak luminosities between those of supernovae (SNe) and superluminous SNe ( M peak ≈ −20)—one discovered and followed by the Palomar Transient Factory (PTF) and three by the Supernova Legacy Survey. The light curves resemble those of SN 2011kl, recently shown to be associated with an ultra-long-duration gamma-ray burst (GRB), though no GRB was seen to accompany our SNe. The rapid rise to a luminous peak places these events in a unique part of SN phase space, challenging standard SN emission mechanisms. Spectra of the PTF event formally classify it as an SN II due to broad H α emission, but an unusual absorption feature, which can be interpreted as either high velocity H α (though deeper than in previously known cases) or Si ii (as seen in SNe Ia), is also observed. We find that existing models of white dwarf detonations, CSM interaction, shock breakout in a wind (or steeper CSM), and magnetar spin down cannot readily explain the observations. We consider the possibility that a “Type 1.5 SN” scenario could be the origin of our events. More detailed models for these kinds of transients and more constraining observations of future such events should help to better determine their nature.

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)0.001
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.609
Threshold uncertainty score0.675

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
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 integrity0.0000.001
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 head0.017
GPT teacher head0.239
Teacher spread0.222 · 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

Citations153
Published2016
Admission routes2
Has abstractyes

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