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Record W2040238702 · doi:10.1093/mnras/stu2297

The JCMT Gould Belt Survey: constraints on prestellar core properties in Orion A North

2015· article· en· W2040238702 on OpenAlexaff
C. Salji, John Richer, Jane Buckle, J. Hatchell, Helen Kirk, S. F. Beaulieu, David Berry, H. Broekhoven-Fiene, M. J. Currie, Michel Fich, Tim Jenness, Doug Johnstone, J. C. Mottram, D. Nutter, Kate Pattle, J. E. Pineda, C. Quinn, S. Tisi, S. Walker-Smith, 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, E. Drabek-Maunder, A. Duarte-Cabral, Jason Fiege, Per Friberg, Rachel Friesen, G. A. Fuller, Sarah Graves, J. S. Greaves, J. Gregson, W. S. Holland, G. Joncas, J. M. Kirk, L. B. G. Knee, Steve Mairs, K. A. Marsh, Brenda C. Matthews, G. H. Moriarty‐Schieven, J. M. C. Rawlings, D. Robertson, 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 ManitobaUniversity of AlbertaUniversité LavalUniversité de MontréalCentre for Research in Astrophysics of QuébecUniversity of VictoriaUniversity of WaterlooHerzberg Institute of Astrophysics
FundersScience and Technology Facilities Council
KeywordsPhysicsAstrophysicsOrion NebulaInitial mass functionStar formationMolecular cloudSolar massStars

Abstract

fetched live from OpenAlex

We employ SCUBA-2 (Submillimetre Common-User Bolometer Array 2) observations of the Orion A North molecular cloud to derive column density and temperature maps. We apply a novel, Hessian-based structural identification algorithm for detection of prestellar cores to these data, allowing for automated generation of the prestellar mass function. The resulting mass function is observed to peak at |$1.39^{+0.18}_{-0.19}$| M⊙, indicating a star-forming efficiency lower limit of ∼14 per cent when compared with the Orion nebula Cluster initial mass function (IMF) peak. Additionally, the prestellar mass function is observed to decay with a high-mass power-law exponent |$\alpha =2.53^{+0.16}_{-0.14}$|⁠, indicating approximate functional similarity with the Salpeter IMF (α = 2.35). This result, when combined with the results of previous investigations suggests a regional dependence of the star-forming efficiency.

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 score0.055
Threshold uncertainty score0.109

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
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 head0.033
GPT teacher head0.229
Teacher spread0.195 · 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

Citations32
Published2015
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical SocietySame topicAstrophysics and Star Formation StudiesFrench-language works237,207