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Record W4213209574 · doi:10.1051/0004-6361/202141307

The LOFAR Two-metre Sky Survey Deep fields

2022· article· en· W4213209574 on OpenAlexfundno aff
I. McCheyne, S. Oliver, M. Sargent, R. Kondapally, D. J. B. Smith, P. Haskell, K. J. Duncan, P. N. Best, J. Sabater, Matteo Bonato, G. Calistro Rivera, R. K. Cochrane, M. C. Campos Varillas, Peter D. Hurley, S. K. Leslie, K. Małek, M. Magliocchetti, I. Prandoni, S. Read, H. J. A. Röttgering, Cyril Tasse, M. Vaccari, L. Wang

Bibliographic record

VenueAstronomy and Astrophysics · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersFP7 International CooperationScience and Technology Facilities CouncilObservatoire de Paris, Université de Recherche Paris Sciences et LettresCentre National de la Recherche ScientifiqueBundesministerium für Bildung und ForschungNarodowe Centrum NaukiInstitut sur la Nutrition et les Aliments FonctionnelsMinisterium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-WestfalenUniversité d'OrléansMinistero degli Affari Esteri e della Cooperazione InternazionaleMax-Planck-GesellschaftNederlandse Organisatie voor Wetenschappelijk OnderzoekNational Science FoundationScience Foundation IrelandSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
KeywordsPhysicsLOFARAstrophysicsJanskyRedshiftSkyGalaxyAstronomyLuminosityQuasarInfraredStellar massStar formationRadio telescopeRadio galaxy

Abstract

fetched live from OpenAlex

The far-infrared radio correlation (FIRC) is one of the strongest correlations in astronomy, yet a model that explains this comprehensively does not exist. The new LOFAR all Sky Survey (LoTSS) deep field, ELAIS-N1, allows exploration of this relation in previously unexplored regions of parameter space of radio frequency (150 MHz), luminosity (L150 < 1024.7), redshift (z ∼ 1), and stellar mass M* < 1011.4. We present accurate deblended far-infrared (FIR) flux measurements with robust errors at 24, 100, 160, 250, 350, and 500 μm from Spitzer and the Herschel Space Observatory using XID+. We find that the FIRC has a strong mass dependence, the evolution of which takes the form qTIR(M*) = (2.00 ± 0.01)+(−0.22 ± 0.02)(log(M/M*)−10.05). This matches recent findings in regards to the star formation rate–radio luminosity relation at 150 MHz and results from radio observations in COSMOS at 1.4 GHz with the Jansky Very Large Array (JVLA). Our results provide tighter constraints on the low-redshift end of the FIRC and at lower frequency than the COSMOS observations. In addition, we find a mild evolution with redshift, with a best fit relation qTIR(z) = (1.94 ± 0.01)(1 + z)−0.04 ± 0.01. This evolution is shallower than that suggested by previous results at 150 MHz with the differences explained by the fact that previous studies did not account for the mass dependence. Finally, we present deblended FIR fluxes for 79 609 galaxies across the LoTSS deep fields: Boötes, ELAIS-N1, and Lockman Hole.

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)0.001
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 score0.016
Threshold uncertainty score0.032

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0080.004

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 head0.006
GPT teacher head0.198
Teacher spread0.192 · 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

Citations12
Published2022
Admission routes1
Has abstractyes

Explore more

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