MétaCan
Menu
Back to cohort
Record W1985697011 · doi:10.1088/0004-637x/698/1/808

POLYYNES AND INTERSTELLAR CARBON NANOPARTICLES

2009· article· en· W1985697011 on OpenAlexaff
W. W. Duley, Anming Hu

Bibliographic record

VenueThe Astrophysical Journal · 2009
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of Waterloo
Fundersnot available
KeywordsCarbon fibersMoleculePhysicsCarbon NanoparticlesInterstellar mediumInfraredAbsorption (acoustics)AstrochemistryCarbon chainNanoparticleSpectral lineInfrared spectroscopyAbsorption spectroscopyPhotochemistryAstrophysicsMaterials scienceChemistryAstronomyOrganic chemistryComposite numberOpticsGalaxyComposite material

Abstract

fetched live from OpenAlex

Laboratory experiments show that long-chain polyyne molecules are often components of the type of carbon nanoparticle (CNP) that can be associated with the infrared (IR) emission bands attributed to polycyclic aromatic hydrocarbons (PAHs). These molecules are attached to peripheral sites on PAH molecules and have in excess of six carbon atoms. IR spectra of CNPs containing a variety of sp-bonded carbon chains in conjunction with PAH groups are reported in this paper. We find that polyyne side-chains produce several notable spectral features in the 4.3 and 5.7 μm (2300–1750 cm −1 ) range, some of which may be present in interstellar emission. A deeper search for these features in absorption or emission in interstellar sources would indicate if polyyne chains are commonly attached to PAH emitters.

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)0.000
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.001
Threshold uncertainty score0.004

Distilled classifier scores by category (both heads)

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 science0.0000.000
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 head0.007
GPT teacher head0.222
Teacher spread0.214 · 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

Citations37
Published2009
Admission routes1
Has abstractyes

Explore more

Same venueThe Astrophysical JournalSame topicAstrophysics and Star Formation StudiesFrench-language works237,207