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Record W2059294377 · doi:10.1093/mnras/stv438

The JCMT Gould Belt Survey: SCUBA-2 observations of circumstellar discs in L 1495

2015· article· en· W2059294377 on OpenAlexafffund
Jane Buckle, E. Drabek-Maunder, J. S. Greaves, John Richer, Brenda C. Matthews, Doug Johnstone, Helen Kirk, S. F. Beaulieu, David Berry, H. Broekhoven-Fiene, M. J. Currie, Michel Fich, J. Hatchell, Tim Jenness, J. C. Mottram, D. Nutter, Kate Pattle, J. E. Pineda, C. Salji, S. Tisi, James Di Francesco, M. R. Hogerheijde, D. Ward–Thompson, Pierre Bastien, H. M. Butner, Michael Chun-Yuan Chen, A. Chrysostomou, Simon Coudé, C. J. Davis, A. Duarte-Cabral, Per Friberg, Rachel Friesen, G. A. Fuller, Sarah Graves, J. Gregson, W. S. Holland, G. Joncas, J. M. Kirk, L. B. G. Knee, Steve Mairs, K. A. Marsh, G. H. Moriarty‐Schieven, J. M. C. Rawlings, Erik Rosolowsky, D. Rumble, Sarah Sadavoy, H. Thomas, N. F. H. Tothill, S. Viti, G. J. White, C. D. Wilson, J. G. A. Wouterloot, J. Yates, Ming Zhu

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2015
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsMcMaster UniversityCanadian Institute for Theoretical AstrophysicsUniversity of TorontoUniversity of AlbertaUniversité LavalUniversité de MontréalCentre for Research in Astrophysics of QuébecUniversity of VictoriaUniversity of WaterlooHerzberg Institute of Astrophysics
FundersScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaNederlandse Organisatie voor Wetenschappelijk OnderzoekCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationNational Science Foundation
KeywordsJames Clerk Maxwell TelescopePhysicsAstrophysicsBolometerWavelengthStarsOpacityAstronomyStellar classificationBrown dwarfTelescopeStellar massStar formationOptics

Abstract

fetched live from OpenAlex

We present 850 and 450 μm data from the James Clerk Maxwell Telescope (JCMT) Gould Belt Survey obtained with Submillimetre Common-User Bolometer Array 2 (SCUBA-2) and characterize the dust attributes of Class I, Class II and Class III disc sources in L 1495. We detect 23 per cent of the sample at both wavelengths, with the detection rate decreasing through the Classes from I to III. The median disc mask is 1.6 × 10−3 M⊙, and only 7 per cent of Class II sources have disc masses larger than 20 Jupiter masses. We detect a higher proportion of discs towards sources with stellar hosts of spectral type K than spectral type M. Class II discs with single stellar hosts of spectral type K have higher masses than those of spectral type M, supporting the hypothesis that higher mass stars have more massive discs. Variations in disc masses calculated at the two wavelengths suggest that there may be differences in dust opacity and/or dust temperature between discs with hosts of spectral types K to those with spectral type M.

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 score0.047
Threshold uncertainty score0.094

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0030.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
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 head0.031
GPT teacher head0.237
Teacher spread0.206 · 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

Citations28
Published2015
Admission routes2
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicAstrophysics and Star Formation Studies→French-language works237,207→