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Record W2747083677 · doi:10.1017/pasa.2017.36

The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array

2017· article· en· W2747083677 on OpenAlexafffund
E. Lenc, C. S. Anderson, N. Barry, Judd D. Bowman, Iver H. Cairns, J. S. Farnes, B. M. Gaensler, G. Heald, M. Johnston‐Hollitt, D. L. Kaplan, C. Lynch, Patrick McCauley, D. A. Mitchell, John Morgan, M. F. Morales, Tara Murphy, A. R. Offringa, S. M. Ord, B. Pindor, C. J. Riseley, E. M. Sadler, C. Sobey, M. Sokołowski, Ian Sullivan, S. P. O’Sullivan, Xiaohui Sun, S. E. Tremblay, Cathryn M. Trott, R. B. Wayth

Bibliographic record

VenuePublications of the Astronomical Society of Australia · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicRadio Astronomy Observations and Technology
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
FundersNatural Sciences and Engineering Research Council of CanadaUniversity of TorontoCanada Research ChairsAstronomy Australia LimitedCurtin University of TechnologyAustralian GovernmentCommonwealth Scientific and Industrial Research Organisation
KeywordsPolarimetryPhysicsFaraday effectPulsarRemote sensingExoplanetIntergalactic travelAstronomyIonosphereFaraday cageOpticsStarsGeologyMagnetic fieldGalaxy

Abstract

fetched live from OpenAlex

Abstract We present techniques developed to calibrate and correct Murchison Widefield Array low-frequency (72–300 MHz) radio observations for polarimetry. The extremely wide field-of-view, excellent instantaneous (u,v)-coverage and sensitivity to degree-scale structure that the Murchison Widefield Array provides enable instrumental calibration, removal of instrumental artefacts, and correction for ionospheric Faraday rotation through imaging techniques. With the demonstrated polarimetric capabilities of the Murchison Widefield Array, we discuss future directions for polarimetric science at low frequencies to answer outstanding questions relating to polarised source counts, source depolarisation, pulsar science, low-mass stars, exoplanets, the nature of the interstellar and intergalactic media, and the solar environment.

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)0.006
metaresearch head score (Gemma)0.008
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: Methods · Consensus signal: Methods
Teacher disagreement score0.006
Threshold uncertainty score0.033

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0060.008
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.003
Scholarly communication0.0020.004
Open science0.0010.002
Research integrity0.0010.003
Insufficient payload (model declined to judge)0.0020.002

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 head0.048
GPT teacher head0.295
Teacher spread0.247 · 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
GenreMethods

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

Citations69
Published2017
Admission routes2
Has abstractyes

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Same venuePublications of the Astronomical Society of AustraliaSame topicRadio Astronomy Observations and TechnologyFrench-language works237,207