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Record W4288604938 · doi:10.1051/0004-6361/201833893

Radio-loud AGN in the first LoTSS data release

2018· article· en· W4288604938 on OpenAlex
M. J. Hardcastle, W. L. Williams, P. N. Best, J. H. Croston, K. J. Duncan, H. J. A. Röttgering, J. Sabater, T. W. Shimwell, C. Tasse, J. R. Callingham, R. K. Cochrane, F. de Gasperin, G. Gürkan, M. J. Jarvis, V. H. Mahatma, G. K. Miley, B. Mingo, S. Mooney, L. K. Morabito, S. P. O’Sullivan, I. Prandoni, A. Shulevski, D. J. B. Smith

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

fundA Canadian funder is recorded on the work.
no affNo Canadian affiliation: this work is invisible to an affiliation-only frame.
No Canadian affiliation. An affiliation-only frame, the usual design, would never have seen this work. It is one of the works that make the case for inverting the frame.

Bibliographic record

VenueAstronomy and Astrophysics · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersLos Alamos National LaboratoryPlanetary Science DivisionSmithsonian Astrophysical ObservatoryLawrence Berkeley National LaboratoryJet Propulsion LaboratoryCommonwealth Scientific and Industrial Research OrganisationEötvös Loránd TudományegyetemNederlandse Organisatie voor Wetenschappelijk OnderzoekDeutsche ForschungsgemeinschaftUniversité d'OrléansBundesministerium für Bildung und ForschungNational Central UniversityBrookhaven National LaboratoryCentre National de la Recherche ScientifiqueMax-Planck-GesellschaftObservatoire de Paris, Université de Recherche Paris Sciences et LettresMinisterium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-WestfalenQueen's University BelfastOffice of ScienceMax-Planck-Institut für AstronomieUniversity of HertfordshireQueen's UniversityUniversity of EdinburghDurham UniversityScience and Technology Facilities CouncilYork UniversityUniversity of PortsmouthNew Mexico State UniversityAssociated UniversitiesSpace Telescope Science InstituteCarnegie Mellon UniversityIrish Research CouncilUniversity of ArizonaCollege of Engineering, Michigan State UniversityUniversity of California, Los AngelesUniversity of WashingtonPrinceton UniversityAlfred P. Sloan FoundationJohns Hopkins UniversityYale UniversityU.S. Department of EnergySmithsonian InstitutionNational Radio Astronomy ObservatoryHarvard UniversityOhio State UniversityHintze Family Charitable FoundationCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationVanderbilt UniversityScience Mission DirectorateScience Foundation IrelandNational Science Foundation
KeywordsPhysicsAstrophysicsAstronomy

Abstract

fetched live from OpenAlex

We constructed a sample of 23 344 radio-loud active galactic nuclei (RLAGN) from the catalogue derived from the LOFAR Two-Metre Sky Survey (LoTSS) survey of the HETDEX Spring field. Although separating AGN from star-forming galaxies remains challenging, the combination of spectroscopic and photometric techniques we used gives us one of the largest available samples of candidate RLAGN. We used the sample, combined with recently developed analytical models, to investigate the lifetime distribution of RLAGN. We show that large or giant powerful RLAGN are probably the old tail of the general RLAGN population, but that the low-luminosity RLAGN candidates in our sample, many of which have sizes < 100 kpc, either require a very different lifetime distribution or have different jet physics from the more powerful objects. We then used analytical models to develop a method of estimating jet kinetic powers for our candidate objects and constructed a jet kinetic luminosity function based on these estimates. These values can be compared to observational quantities, such as the integrated radiative luminosity of groups and clusters, and to the predictions from models of RLAGN feedback in galaxy formation and evolution. In particular, we show that RLAGN in the local Universe are able to supply all the energy required per comoving unit volume to counterbalance X-ray radiative losses from groups and clusters and thus prevent the hot gas from cooling. Our computation of the kinetic luminosity density of local RLAGN is in good agreement with other recent observational estimates and with models of galaxy formation.

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.

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Other design · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.927
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.013
GPT teacher head0.221
Teacher spread0.207 · 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