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Record W2090094926 · doi:10.1051/0004-6361/201116466

<i>Planck</i>early results. XV. Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources

2011· article· en· W2090094926 on OpenAlexaff
Juha Aatrokoski, P. A. R. Ade, N. Aghanim, H. D. Aller, M. F. Aller, E. Angelakis, M. Arnaud, M. Ashdown, J. Aumont, C. Baccigalupi, A. Balbi, A. J. Banday, R. B. Barreiro, J. G. Bartlett, E. Battaner, K. Benabed, A. Benoı̂t, A. Berdyugin, J.-P. Bernard, M. Bersanelli, R. Bhatia, A. Bonaldi, L. Bonavera, J. R. Bond, J. Borrill, F. R. Bouchet, M. Bucher, C. Burigana, D. N. Burrows, P. Cabella, M. Capalbi, B. Cappellini, J.-F. Cardoso, A. Catalano, E. Cavazzuti, L. Cayón, A. Challinor, A. Chamballu, Ranga‐Ram Chary, L.-Y Chiang, P. R. Christensen, D. L. Clements, S. Colafrancesco, S. Colombi, F. Couchot, A. Coulais, S. Cutini, F. Cuttaia, L. Danese, R. D. Davies, R. J. Davis, P. de Bernardis, G. de Gasperis, A. de Rosa, G. de Zotti, J.‐M. Delouis, C. Dickinson, H. Dole, S. Donzelli, O. Doré, U. Dörl, M. Douspis, X. Dupac, G. Efstathiou, T. A. Enßlin, F. Finelli⋆, O. Forni, M. Frailis, E. Franceschi, L. Fuhrmann, S. Galeotta, K. Ganga, F. Gargano, D. Gasparrini, N. Gehrels, M. Giard, G. Giardino, N. Giglietto, P. Giommi, F. Giordano, Y. Giraud–Héraud, J. González-Nuevo, K. M. Górski, S. Gratton, A. Gregorio, A. Gruppuso, D. L. Harrison, S. Henrot–Versillé, D. Herranz, S. R. Hildebrandt, E. Hivon, W. A. Holmes, W. Hovest, R. J. Hoyland, K. M. Huffenberger, A. H. Jaffe, M. Juvela, E. Keihänen, R. Keskitalo, O. G. King, T. S. Kisner, R. Kneißl, L. Knox, T. P. Krichbaum, H. Kurki‐Suonio, G. Lagache, A. Lähteenmäki, J.‐M. Lamarre, A. Lasenby, R. J. Laureijs, N. Lavonen, C. R. Lawrence, S. Leach, R. Leonardi, J. León-Tavares, M. Linden-Vørnle, E. Lindfors, M. López-Caniego, P. M. Lubin, J. F. Macías–Pérez, B. Maffei, D. Maino, N. Mandolesi, Robert G. Mann, M. Maris, E. Martínez-González, S. Masi, M. Massardi, S. Matarrese, F. Matthai, W. Max-Moerbeck, M. N. Mazziotta, P. Mazzotta, A. Melchiorri, L. Mendes, A. Mennella, P. F. Michelson, М. Г. Мингалиев, S. Mitra, M.-A. Miville-Deschênes, A. Moneti, C. Monte, L. Montier, G. Morgante, D. Mortlock, D. Munshi, A. Murphy, P. Naselsky, P. Natoli, I. Nestoras, C. B. Netterfield, E. Nieppola, K. Nilsson, H. U. Nørgaard-Nielsen, F. Noviello, D. Novikov, I. Novikov, I. J. O’Dwyer, S. Osborne, F. Pajot, B. Partridge, F. Pasian, G. Patanchon, V. Pavlidou, T. J. Pearson, O. Perdereau, L. Perotto, M. Perri, F. Perrotta, F. Piacentini, M. Piat, S. Plaszczynski, P. Platania, É. Pointecouteau, G. Polenta, N. Ponthieu, T. Poutanen, G. Prézeau, P. Procopio, S. Prunet, J.‐L. Puget, J. P. Rachen, S. Rainò, W. T. Reach, A. C. S. Readhead, R. Rébolo, R. Reeves, M. Reinecke, R. Reinthal, C. Renault, S. Ricciardi, J. L. Richards, T. Riller, D. Riquelme, I. Ristorcelli, G. Rocha, C. Rosset, M. Rowan-Robinson, J. A. Rubiño-Martín, B. Rusholme, J. Saarinen, M. Sandri, Petri Savolainen, D. Scott, M. D. Seiffert, A. Sievers, A. Sillanpää, G. F. Smoot, Yu. V. Sotnikova, Jean‐Luc Starck, M. A. Stevenson, F. Stivoli, V. Stolyarov, R. Sudiwala, J.-F. Sygnet, L. O. Takalo, J. Tammi, J. A. Tauber, L. Terenzi, D. J. Thompson, L. Toffolatti, M. Tomasi, M. Tornikoski, J.–P. Torre, G. Tosti, A. Tramacere, M. Tristram, J. Tuovinen, M. Türler, Mika Turunen, G. Umana, H. Ungerechts, L. Valenziano, E. Valtaoja, J. Varis, F. Verrecchia, P. Vielva, F. Villa, N. Vittorio, B. D. Wandelt, Jianghua Wu, D. Yvon, A. Zacchei, J. A. Zensus, Xin Zhou, A. Zonca

Bibliographic record

VenueAstronomy and Astrophysics · 2011
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of British ColumbiaUniversity of Toronto
FundersJapan Aerospace Exploration AgencyInstitut National de Physique Nucléaire et de Physique des ParticulesScience and Technology Facilities CouncilJet Propulsion LaboratoryInstituto de Astrofísica de CanariasUniversité Paris-SudIstituto Nazionale di Fisica NucleareUniversité de GenèveUniversidad de CantabriaUniversitetet i OsloIstituto Nazionale di AstrofisicaINAF - Osservatorio Astrofisico di CataniaMinisterio de Ciencia e InnovaciónCentre National de la Recherche ScientifiqueNational Key Research and Development Program of ChinaEuropean Southern ObservatoryU.S. Department of EnergyNational Radio Astronomy ObservatoryVetenskapsrådetCalifornia Institute of TechnologyTekesFundação para a Ciência e a TecnologiaCentre National d’Etudes SpatialesMinistry of Education, Culture, Sports, Science and TechnologyNational Science FoundationScience Foundation IrelandAcademy of FinlandAcademia SinicaCommonwealth Scientific and Industrial Research OrganisationHigh Energy Accelerator Research OrganizationMinistério da Ciência, Tecnologia e Ensino SuperiorUK Space AgencyAgenzia Spaziale ItalianaImperial College LondonInstituto de Física de CantabriaMax-Planck-GesellschaftUniversity of MichiganChina Scholarship CouncilNational Aeronautics and Space AdministrationAssociated UniversitiesInstitut national de recherche en informatique et en automatique (INRIA)
KeywordsPhysicsAstrophysicsPlanckSpectral lineAstronomySpectral energy distribution

Abstract

fetched live from OpenAlex

Spectral energy distributions (SEDs) and radio continuum spectra are presented for a northern sample of 104 extragalactic radio sources, based on the Planck Early Release Compact Source Catalogue (ERCSC) and simultaneous multifrequency data. The nine Planck frequencies, from 30 to 857 GHz, are complemented by a set of simultaneous observations ranging from radio to gamma-rays. This is the first extensive frequency coverage in the radio and millimetre domains for an essentially complete sample of extragalactic radio sources, and it shows how the individual shocks, each in their own phase of development, shape the radio spectra as they move in the relativistic jet. The SEDs presented in this paper were fitted with second and third degree polynomials to estimate the frequencies of the synchrotron and inverse Compton (IC) peaks, and the spectral indices of low and high frequency radio data, including the Planck ERCSC data, were calculated. SED modelling methods are discussed, with an emphasis on proper, physical modelling of the synchrotron bump using multiple components. Planck ERCSC data also suggest that the original accelerated electron energy spectrum could be much harder than commonly thought, with power-law index around 1.5 instead of the canonical 2.5. The implications of this are discussed for the acceleration mechanisms effective in blazar shocks. Furthermore in many cases the Planck data indicate that gamma-ray emission must originate in the same shocks that produce the radio emission.

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)0.000
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: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.519
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
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 head0.007
GPT teacher head0.173
Teacher spread0.166 · 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 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

Citations119
Published2011
Admission routes1
Has abstractyes

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