MétaCan
Menu
Back to cohort
Record W3089158549 · doi:10.1093/mnras/staa3023

Square Kilometre Array Science Data Challenge 1: analysis and results

2020· article· en· W3089158549 on OpenAlexaff
Anna Bonaldi, Tao An, M. Brüggen, Sandra Burkutean, Bruno Coelho, Hadis Goodarzi, Philippa Hartley, Pritpal Sandhu, Chonghao Wu, Lei Yu, Mohammad H. Zhoolideh Haghighi, Sonia Antón, Zahra Bagheri, Domingos Barbosa, João Paulo Barraca, Dzianis Bartashevich, Miguel Bergano, Matteo Bonato, J. Brand, F. de Gasperin, A. Giannetti, Richard Dodson, Pankaj Jain, Sumit Jaiswal, Baoqiang Lao, Bin Liu, Elisabetta Liuzzo, Yi Lu, Vesna Lukic, D. Maia, N. Marchili, M. Massardi, P. Mohan, Joana Morgado, Mohit Panwar, P. Prabhakar, V. A. R. M. Ribeiro, K. L. J. Rygl, V Sabz Ali, Elham Saremi, E. Schisano, Somayeh Sheikhnezami, Alexander Wong, O. Ivy Wong

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicRadio Astronomy Observations and Technology
Canadian institutionsUniversity of Waterloo
FundersFuel Cell Technologies ProgramPrograma Operacional Temático Factores de CompetitividadeMinistério da Ciência, Tecnologia e Ensino Superior
KeywordsPhysicsKilometerSquare (algebra)AstronomyAstrophysicsGeometry

Abstract

fetched live from OpenAlex

ABSTRACT As the largest radio telescope in the world, the Square Kilometre Array (SKA) will lead the next generation of radio astronomy. The feats of engineering required to construct the telescope array will be matched only by the techniques developed to exploit the rich scientific value of the data. To drive forward the development of efficient and accurate analysis methods, we are designing a series of data challenges that will provide the scientific community with high-quality data sets for testing and evaluating new techniques. In this paper, we present a description and results from the first such Science Data Challenge 1 (SDC1). Based on SKA MID continuum simulated observations and covering three frequencies (560, 1400, and 9200 MHz) at three depths (8, 100, and 1000 h), SDC1 asked participants to apply source detection, characterization, and classification methods to simulated data. The challenge opened in 2018 November, with nine teams submitting results by the deadline of 2019 April. In this work, we analyse the results for eight of those teams, showcasing the variety of approaches that can be successfully used to find, characterize, and classify sources in a deep, crowded field. The results also demonstrate the importance of building domain knowledge and expertise on this kind of analysis to obtain the best performance. As high-resolution observations begin revealing the true complexity of the sky, one of the outstanding challenges emerging from this analysis is the ability to deal with highly resolved and complex sources as effectively as the unresolved source population.

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)0.013
metaresearch head score (Gemma)0.036
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.016
Threshold uncertainty score0.068

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0130.036
Meta-epidemiology (narrow)0.0020.000
Meta-epidemiology (broad)0.0020.002
Bibliometrics0.0030.003
Science and technology studies0.0020.001
Scholarly communication0.0040.003
Open science0.0030.004
Research integrity0.0030.004
Insufficient payload (model declined to judge)0.0030.006

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 head0.024
GPT teacher head0.237
Teacher spread0.213 · 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

Citations52
Published2020
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical SocietySame topicRadio Astronomy Observations and TechnologyFrench-language works237,207