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Record W2430862193 · doi:10.1051/0004-6361/201527780

Planck intermediate results XLV. Radio spectra of northern extragalactic radio sources

2016· article· en· W2430862193 on OpenAlexaff
N. Aghanim, H. D. Aller, M. F. Aller, M. Arnaud, J. Aumont, C. Baccigalupi, A. J. Banday, R. B. Barreiro, N. Bartolo, E. Battaner, K. Benabed, A. Benoit-Lévy, J.-P. Bernard, M. Bersanelli, P. Bielewicz, A. Bonaldi, L. Bonavera, J. R. Bond, J. Borrill, F. R. Bouchet, C. Burigana, Erminia Calabrese, A. Catalano, H. C. Chiang, P. R. Christensen, D. L. Clements, L. P. L. Colombo, F. Couchot, B. P. Crill, A. Curto, F. Cuttaia, L. Danese, R. D. Davies, R. J. Davis, P. de Bernardis, A. de Rosa, G. de Zotti, C. Dickinson, J. M. Diego, H. Dole, S. Donzelli, O. Doré, A. Ducout, X. Dupac, G. Efstathiou, F. Elsner, H. K. Eriksen, F. Finelli⋆, O. Forni, M. Frailis, A. A. Fraisse, E. Franceschi, S. Galeotta, S. Galli, K. Ganga, M. Giard, Y. Giraud–Héraud, E. Gjerløw, J. González-Nuevo, K. M. Górski, A. Gruppuso, Mark Gurwell, F. K. Hansen, D. L. Harrison, S. Henrot–Versillé, C. Hernández-Monteagudo, S. R. Hildebrandt, A. Hornstrup, T. Hovatta, W. Hovest, K. M. Huffenberger, G. Hurier, A. H. Jaffe, T. R. Jaffe, E. Järvelä, E. Keihänen, R. Keskitalo, T. S. Kisner, R. Kneißl, J. Knoche, M. Kunz, H. Kurki‐Suonio, A. Lähteenmäki, J.-M. Lamarre, A. Lasenby, M. Lattanzi, Charles R. Lawrence, R. Leonardi, F. Levrier, M. Liguori, P. B. Lilje, M. Linden-Vørnle, M. López-Caniego, P. M. Lubin, J. F. Macías–Pérez, B. Maffei, D. Maino, N. Mandolesi, M. Maris, P. G. Martin, E. Martínez-González, S. Masi, S. Matarrese, W. Max-Moerbeck, P. R. Meinhold, A. Melchiorri, A. Mennella, M. Migliaccio, M.-A. Miville-Deschênes, A. Moneti, L. Montier, G. Morgante, D. Mortlock, D. Munshi, J. A. Murphy, F. Nati, P. Natoli, E. Nieppola, F. Noviello, D. Novikov, I. Novikov, L. Pagano, F. Pajot, D. Paoletti, Bruce Partridge, F. Pasian, T. J. Pearson, O. Perdereau, L. Perotto, V. Pettorino, F. Piacentini, M. Piat, E. Pierpaoli, S. Plaszczynski, É. Pointecouteau, G. Polenta, G. W. Pratt, Venkatessh Ramakrishnan, Elizaveta Rastorgueva-Foi, M. Reinecke, M. Remazeilles, C. Renault, A. Renzi, J. L. Richards, I. Ristorcelli, G. Rocha, M. Rossetti, G. Roudier, J. A. Rubiño-Martín, B. Rusholme, M. Sandri, М. Савелайнен, G. Savini, D. Scott, Yu. V. Sotnikova, V. Stolyarov, R. Sunyaev, D. Sutton, A.-S. Suur-Uski, J.-F. Sygnet, J. Tammi, J. A. Tauber, L. Terenzi, L. Toffolatti, M. Tomasi, M. Tornikoski, M. Tristram, M. Türler, L. Valenziano, J. Väliviita, E. Valtaoja, P. Vielva, L. A. Wade, A. E. Wehrle, I. K. Wehus, D. Yvon, A. Zacchei, A. Zonca

Bibliographic record

VenueORCA Online Research @Cardiff (Cardiff University) · 2016
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of British ColumbiaUniversity of Toronto
FundersFundação para a Ciência e a TecnologiaSmithsonian Astrophysical ObservatoryInstitut National de Physique Nucléaire et de Physique des ParticulesMinistério da Ciência, Tecnologia e Ensino SuperiorCentre National de la Recherche ScientifiqueScience and Technology Facilities CouncilTekesCentre National d’Etudes SpatialesPartnership for Advanced Computing in Europe AISBLAcademia SinicaNational Science FoundationEuropean Space AgencyKazan Federal UniversityChina Scholarship CouncilNational Aeronautics and Space AdministrationMax-Planck-GesellschaftUK Space AgencySmithsonian InstitutionScience Foundation Ireland
KeywordsPhysicsAstrophysicsPlanckSpectral indexSpectral lineAstronomyRadio spectrumWavelengthRadio frequency

Abstract

fetched live from OpenAlex

Continuum spectra covering centimetre to submillimetre wavelengths are presented for a northern sample of 104 extragalactic radio sources, mainly active galactic nuclei, based on four-epoch Planck data. The nine Planck frequencies, from 30 to 857 GHz, are complemented by a set of simultaneous ground-based radio observations between 1.1 and 37 GHz. The single-survey Planck data confirm that the flattest high-frequency radio spectral indices are close to zero, indicating that the original accelerated electron energy spectrum is much harder than commonly thought, with power-law index around 1.5 instead of the canonical 2.5. The radio spectra peak at high frequencies and exhibit a variety of shapes. For a small set of low-z sources, we find a spectral upturn at high frequencies, indicating the presence of intrinsic cold dust. Variability can generally be approximated by achromatic variations, while sources with clear signatures of evolving shocks appear to be limited to the strongest outbursts.

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 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)0.001
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: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.574
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.001
Science and technology studies0.0000.001
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.001
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 head0.022
GPT teacher head0.254
Teacher spread0.232 · 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 teacher head, not a consensus.

Study designNot applicable
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

Citations19
Published2016
Admission routes1
Has abstractyes

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Same venueORCA Online Research @Cardiff (Cardiff University)Same topicAstrophysics and Cosmic PhenomenaFrench-language works237,207