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Record W2146390124 · doi:10.1093/mnras/stv1833

The JCMT Plane Survey: early results from the ℓ = 30° field

2015· article· en· W2146390124 on OpenAlexaff
T. J. T. Moore, R. Plume, M. A. Thompson, Harriet Parsons, J. S. Urquhart, David Eden, J. T. Dempsey, L. K. Morgan, H. Thomas, J. Buckle, Christopher M. Brunt, H. M. Butner, D. Carretero, A. Chrysostomou, H. M. deVilliers, Michel Fich, M. G. Hoare, G. Manser, J. C. Mottram, C. Natário, Fernando A. Olguin, N. Peretto, D. Polychroni, R. O. Redman, A. J. Rigby, C. Salji, L. J. Summers, David Berry, M. J. Currie, Tim Jenness, M. Pestalozzi, A. Traficante, Pierre Bastien, J. Difrancesco, C. J. Davis, A. Evans, Per Friberg, G. A. Fuller, A. G. Gibb, S. J. Gibson, T. Hill, Doug Johnstone, G. Joncas, Steven N. Longmore, S. L. Lumsden, P. G. Martin, Q. Nguyê ̃n Lu'o’ng, J. E. Pineda, Cormac Purcell, John Richer, G. Schieven, R. F. Shipman, M. Spaans, A. R. Taylor, S. Viti, B. Weferling, G. J. White, Ming Zhu

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2015
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of TorontoUniversity of British ColumbiaHerzberg Institute of AstrophysicsUniversity of WaterlooUniversité LavalUniversité de MontréalCentre for Research in Astrophysics of QuébecUniversity of VictoriaUniversity of Calgary
FundersScience and Technology Facilities Council
KeywordsPhysicsAstrophysicsGalactic planeJames Clerk Maxwell TelescopeFlux (metallurgy)TelescopeGalaxyBrightnessAstronomySource countsStar formationRedshift

Abstract

fetched live from OpenAlex

We present early results from the JCMT (James Clerk Maxwell Telescope) Plane Survey (JPS), which has surveyed the northern inner Galactic plane between longitudes ℓ = 7° and ℓ = 63° in the 850-μm continuum with SCUBA-2 (Submm Common-User Bolometer Array 2), as part of the JCMT Legacy Survey programme. Data from the ℓ = 30° survey region, which contains the massive-star-forming regions W43 and G29.96, are analysed after approximately 40 per cent of the observations had been completed. The pixel-to-pixel noise is found to be 19 mJy beam−1 after a smooth over the beam area, and the projected equivalent noise levels in the final survey are expected to be around 10 mJy beam−1. An initial extraction of compact sources was performed using the FellWalker method, resulting in the detection of 1029 sources above a 5σ surface-brightness threshold. The completeness limits in these data are estimated to be around 0.2 Jy beam−1 (peak flux density) and 0.8 Jy (integrated flux density) and are therefore probably already dominated by source confusion in this relatively crowded section of the survey. The flux densities of extracted compact sources are consistent with those of matching detections in the shallower APEX (Atacama Pathfinder Experiment) Telescope Large Area Survey of the Galaxy (ATLASGAL) survey. We analyse the virial and evolutionary state of the detected clumps in the W43 star-forming complex and find that they appear younger than the Galactic-plane average.

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)0.001
metaresearch head score (Gemma)0.003
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 score0.091
Threshold uncertainty score0.180

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.003
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0030.004
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.001

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 head0.219
Teacher spread0.202 · 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

Citations61
Published2015
Admission routes1
Has abstractyes

Explore more

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