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Record W3103779440 · doi:10.1051/0004-6361/201833562

The LOFAR Two-metre Sky Survey

2018· article· en· W3103779440 on OpenAlexfundno aff
K. J. Duncan, J. Sabater, H. J. A. Röttgering, M. J. Jarvis, D. J. B. Smith, P. N. Best, J. R. Callingham, R. K. Cochrane, J. H. Croston, M. J. Hardcastle, B. Mingo, L. K. Morabito, D. Nisbet, I. Prandoni, T. W. Shimwell, C. Tasse, G. J. White, W. L. Williams, L. Alegre, K. T. Chyży, G. Gürkan, M. Hoeft, R. Kondapally, A. P. Mechev, G. K. Miley, Dominik J. Schwarz, R. J. van Weeren

Bibliographic record

VenueAstronomy and Astrophysics · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersPlanetary Science DivisionScience and Technology Facilities CouncilObservatoire de Paris, Université de Recherche Paris Sciences et LettresScience Mission DirectorateSmithsonian Astrophysical ObservatoryJet Propulsion LaboratoryEötvös Loránd TudományegyetemDurham UniversityIstituto Nazionale di AstrofisicaMax-Planck-GesellschaftNederlandse Organisatie voor Wetenschappelijk OnderzoekQueen's UniversityUniversity of California, Los AngelesUniversity of HertfordshireMinisterium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-WestfalenCommonwealth Scientific and Industrial Research OrganisationEuropean Research CouncilSeventh Framework ProgrammeGordon and Betty Moore FoundationQueen's University BelfastBundesministerium für Bildung und ForschungMax-Planck-Institut für AstronomieUniversity of EdinburghCentre National de la Recherche ScientifiqueUniversity of OxfordNational Central UniversityUniversité d'OrléansLeverhulme TrustSmithsonian InstitutionHintze Family Charitable FoundationSpace Telescope Science InstituteCalifornia Institute of TechnologyEuropean CommissionLos Alamos National LaboratoryJohns Hopkins UniversityNational Aeronautics and Space AdministrationNational Science Foundation
KeywordsPhysicsLOFARAstrophysicsRedshiftSkyDeclinationQuasarPopulationAstronomyPhotometry (optics)Luminosity functionRadio telescopeGalaxyStars

Abstract

fetched live from OpenAlex

The LOFAR Two-metre Sky Survey (LoTSS) is a sensitive, high-resolution 120–168 MHz survey of the Northern sky. The LoTSS First Data Release (DR1) presents 424 square degrees of radio continuum observations over the HETDEX Spring Field (10h45m00s < right ascension < 15h30m00s and 45°00′00″ < declination < 57°00′00″) with a median sensitivity of 71 μJy beam−1 and a resolution of 6″. In this paper we present photometric redshifts (photo-z) for 94.4% of optical sources over this region that are detected in the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) 3π steradian survey. Combining the Pan-STARRS optical data with mid-infrared photometry from the Wide-field Infrared Survey Explorer, we estimate photo-zs using a novel hybrid photometric redshift methodology optimised to produce the best possible performance for the diverse sample of radio continuum selected sources. For the radio-continuum detected population, we find an overall scatter in the photo-z of 3.9% and an outlier fraction (|zphot−zspec|/(1 + zspec) > 0.15) of 7.9%. We also find that, at a given redshift, there is no strong trend in photo-z quality as a function of radio luminosity. However there are strong trends as a function of redshift for a given radio luminosity, a result of selection effects in the spectroscopic sample and/or intrinsic evolution within the radio source population. Additionally, for the sample of sources in the LoTSS First Data Release with optical counterparts, we present rest-frame optical and mid-infrared magnitudes based on template fits to the consensus photometric (or spectroscopic when available) redshift.

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)0.002
metaresearch head score (Gemma)0.002
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: none
Teacher disagreement score0.018
Threshold uncertainty score0.060

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.002
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0030.002
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0180.015

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 head0.008
GPT teacher head0.211
Teacher spread0.203 · 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

Citations81
Published2018
Admission routes1
Has abstractyes

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