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Record W4225556548 · doi:10.1093/mnras/stab2860

[no title]

2021· article· en· W4225556548 on OpenAlexafffund
Peter Scicluna, F. Kemper, Iain McDonald, S. Srinivasan, Alfonso Trejo, S. H. J. Wallström, J. G. A. Wouterloot, J. Cami, J. S. Greaves, Jinhua He, Do Thi Hoai, Hyosun Kim, Olivia Jones, Hiroko Shinnaga, Christopher Clark, T. E. Dharmawardena, W. S. Holland, Hiroshi Imai, Jacco Th. van Loon, K. M. Menten, R. Wesson, Hannah Chawner, Siyi Feng, Steven Goldman, Fang-Chun Liu, Heather MacIsaac, Jinkui Tang, S. T. Zeegers, Kei Amada, Vallia Antoniou, Ashley Bemis, Martha L. Boyer, S. Chapman, X Chen, S-H Cho, Liyuan Cui, F. Dell’Agli, Per Friberg, S. Fukaya, H Gomez, M. Hadjara, C. A. Haswell, Naomi Hirano, S. Hony, Hideyuki Izumiura, M. Jeste, Xiangqian Jiang, T. Kamiński, N. Keaveney, Jaeheon Kim, K E Kraemer, Y.‐J. Kuan, E. Lagadec, Chin‐Fei Lee, Dong Li, Teng Liu, F. Lykou, Claudia Maraston, J. P. Marshall, M. Matsuura, Masaaki Otsuka, Miyako Oyadomari, Harriet Parsons, Nimesh Patel, E. Peeters, Jun Qiu, S. K. Randall, Gioia Rau, M. P. Redman, A. M. S. Richards, S. Serjeant, Chang-Sheng Shi, G. C. Sloan, M. W. L. Smith, J. A. Toalá, S. Uttenthaler, P. Ventura, Bo Wang, I. Yamamura, Tao-Zhi Yang, Yifeng Yun, Fan Zhang, Yong Zhang, Guoying Zhao, Ming Zhu, A. A. Zijlstra

Bibliographic record

VenuearXiv (Cornell University) · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsDalhousie UniversityMcMaster UniversityWestern University
FundersNatural Sciences and Engineering Research Council of CanadaVlaamse regeringNational Astronomical Observatory of JapanChinese Academy of Sciences South America Center for AstronomyMinistry of Science and Technology, TaiwanNational Research Foundation of KoreaNational Aeronautics and Space AdministrationKorea Astronomy and Space Science InstituteFonds Wetenschappelijk OnderzoekChinese Academy of SciencesAcademia SinicaScience and Technology Facilities CouncilNational Research FoundationGreat Britain Sasakawa FoundationNational Natural Science Foundation of China
KeywordsPhysicsAstrophysicsStarsJames Clerk Maxwell TelescopeAstronomySkyGalactic planeTelescopeBlack-body radiationStar formationOptics

Abstract

fetched live from OpenAlex

The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of $\sim$850 Galactic evolved stars within 3\,kpc at (sub-)mm wavelengths, observed in the CO $J = $ (2$-$1) and (3$-$2) rotational lines, and the sub-mm continuum, using the James Clark Maxwell Telescope and Atacama Pathfinder Experiment. NESS consists of five tiers, based on distances and dust-production rate (DPR). We define a new metric for estimating the distances to evolved stars and compare its results to \emph{Gaia} EDR3. Replicating other studies, the most-evolved, highly enshrouded objects in the Galactic Plane dominate the dust returned by our sources, and we initially estimate a total DPR of $4.7\times 10^{-5}$ M$_\odot$ yr$^{-1}$ from our sample. Our sub-mm fluxes are systematically higher and spectral indices are typically shallower than dust models typically predict. The 450/850 $\mu$m spectral indices are consistent with the blackbody Rayleigh--Jeans regime, suggesting a large fraction of evolved stars have unexpectedly large envelopes of cold dust.

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 categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Other · Consensus signal: none
Teacher disagreement score0.989
Threshold uncertainty score0.000

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 communication0.0000.000
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0110.009

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 head0.039
GPT teacher head0.164
Teacher spread0.124 · 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.

Study designNot applicable
Domainnot available
GenreOther

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

Citations15
Published2021
Admission routes2
Has abstractyes

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