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Record W2101841715 · doi:10.25916/sut.26227760.v1

Science with the Australian square kilometre array pathfinder

2024· article· en· W2101841715 on OpenAlexaff
S. Johnston, M. Bailes, N. Bartel, C. M. Baugh, M. F. Bietenholz, Chris Blake, Róbert Braun, J. C. Brown, Shami Chatterjee, Jeremy Darling, Adam T. Deller, Richard Dodson, P. G. Edwards, R. D. Ekers, S. P. Ellingsen, Ilana Feain, B. M. Gaensler, M. Haverkorn, G. Hobbs, Andrew Hopkins, Carole Jackson, C. James, G. Joncas, V. M. Kaspi, V. A. Kilborn, B. Koribalski, R. Kothes, T. L. Landecker, E. Lenc, J. E. J. Lovell, Jean‐Pierre Macquart, R. N. Manchester, D. Matthews, N. M. McClure‐Griffiths, R. P. Norris, Ue‐Li Pen, Chris Phillips, Chris Power, R. J. Protheroe, E. M. Sadler, B. Schmidt, I. H. Stairs, L. Staveley‐Smith, J. M. Stil, Russ Taylor, S. J. Tingay, A. K. Tzioumis, M. A. Walker, J. V. Wall, M. Wolleben

Bibliographic record

VenueUWA Profiles and Research Repository (University of Western Australia) · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicRadio Astronomy Observations and Technology
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of TorontoUniversity of CalgaryMcGill UniversityUniversité LavalHerzberg Institute of AstrophysicsUniversity of British ColumbiaYork University
Fundersnot available
KeywordsPathfinderRadio telescopeTelescopeObservatoryPhysicsSkyAstronomyRadio astronomyPopulationGalactic astronomyGalaxyRemote sensingComputer scienceGeographyMilky WayLibrary science

Abstract

fetched live from OpenAlex

The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive than any existing radio facility. Most of the key science for the SKA will be addressed through large-area imaging of the Universe at frequencies from a few hundred MHz to a few GHz. The Australian SKA Pathfinder (ASKAP) is a technology demonstrator aimed in the mid-frequency range, and achieves instantaneous wide-area imaging through the development and deployment of phased-array feed systems on parabolic reflectors. The large field-of-view makes ASKAP an unprecedented synoptic telescope that will make substantial advances in SKA key science. ASKAP will be located at the Murchison Radio Observatory in inland Western Australia, one of the most radio-quiet locations on the Earth and one of two sites selected by the international community as a potential location for the SKA. In this paper, we outline an ambitious science program for ASKAP, examining key science such as understanding the evolution, formation and population of galaxies including our own, understanding the magnetic Universe, revealing the transient radio sky and searching for gravitational waves.

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)0.003
metaresearch head score (Gemma)0.004
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.034
Threshold uncertainty score0.068

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.004
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0040.003
Science and technology studies0.0020.001
Scholarly communication0.0030.003
Open science0.0010.004
Research integrity0.0010.002
Insufficient payload (model declined to judge)0.0140.010

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 head0.046
GPT teacher head0.299
Teacher spread0.253 · 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 designNot applicable
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

Citations245
Published2024
Admission routes1
Has abstractyes

Explore more

Same venueUWA Profiles and Research Repository (University of Western Australia)Same topicRadio Astronomy Observations and TechnologyFrench-language works237,207