Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/33049
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Bach, U. | en_US |
dc.contributor.author | RAITERI, Claudia Maria | en_US |
dc.contributor.author | VILLATA, Massimo | en_US |
dc.contributor.author | Fuhrmann, L. | en_US |
dc.contributor.author | BUEMI, CARLA SIMONA | en_US |
dc.contributor.author | Larionov, V.M. | en_US |
dc.contributor.author | LETO, PAOLO | en_US |
dc.contributor.author | Arkharov, G.A.A. | en_US |
dc.contributor.author | Coloma, J.M. | en_US |
dc.contributor.author | DI PAOLA, Andrea | en_US |
dc.contributor.author | DOLCI, Mauro | en_US |
dc.contributor.author | Efimova, N. | en_US |
dc.contributor.author | Forné, E. | en_US |
dc.contributor.author | Ibrahimov, M.A. | en_US |
dc.contributor.author | Hagen-Thorn, V. | en_US |
dc.contributor.author | Konstantinova, T. | en_US |
dc.contributor.author | Kopatskaya, E. | en_US |
dc.contributor.author | LANTERI, Luciano | en_US |
dc.contributor.author | Kurtanidze, O.M. | en_US |
dc.contributor.author | MACCAFERRI, Giuseppe | en_US |
dc.contributor.author | Nikolashvili, M.G. | en_US |
dc.contributor.author | ORLATI, ANDREA | en_US |
dc.contributor.author | Ros, J.A. | en_US |
dc.contributor.author | Tosti, G. | en_US |
dc.contributor.author | TRIGILIO, CORRADO | en_US |
dc.contributor.author | UMANA, Grazia Maria Gloria | en_US |
dc.date.accessioned | 2023-01-24T15:12:31Z | - |
dc.date.available | 2023-01-24T15:12:31Z | - |
dc.date.issued | 2007 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/33049 | - |
dc.description.abstract | Context: Being dominated by non-thermal emission from aligned relativistic jets, blazars allow us to elucidate the physics of extragalactic jets, and, ltimately, how the energy is extracted from the central black hole in radio-loud active galactic nuclei. Aims: Crucial information is provided by broad-band spectral energy distributions (SEDs), their trends with luminosity and correlated multi-frequency variability. With this study we plan to obtain a database of contemporaneous radio-to-optical spectra of a sample of blazars, which are and will be observed by current and future high-energy satellites. Methods: Since December 2004 we are performing a monthly multi-frequency radio monitoring of a sample of 35 blazars at the antennas in Medicina and Noto. Contemporaneous near-IR and optical observations for all our observing epochs are organised. Results: Until June 2006 about 4000 radio measurements and 5500 near-IR and optical measurements were obtained. Most of the sources show significant variability in all observing bands. Here we present the multi-frequency data acquired during the first eighteen months of the project, and construct the SEDs for the best-sampled sources. | en_US |
dc.language.iso | eng | en_US |
dc.title | Multi-frequency monitoring of γ-ray loud blazars I. Light curves and spectral energy distributions | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1051/0004-6361:20066561 | en_US |
dc.identifier.scopus | 2-s2.0-33947186164 | en_US |
dc.identifier.url | https://www.aanda.org/articles/aa/abs/2007/10/aa6561-06/aa6561-06.html | en_US |
dc.identifier.url | http://www.scopus.com/inward/record.url?eid=2-s2.0-33947186164&partnerID=MN8TOARS | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 464 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 175 | en_US |
dc.relation.lastpage | 186 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 26 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTRONOMY & ASTROPHYSICS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2007A&A...464..175B | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.journal.journalissn | 0004-6361 | - |
crisitem.journal.ance | E016240 | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Abruzzo | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.orcid | 0000-0003-1784-2784 | - |
crisitem.author.orcid | 0000-0003-1743-6946 | - |
crisitem.author.orcid | 0000-0002-7288-4613 | - |
crisitem.author.orcid | 0000-0003-4864-2806 | - |
crisitem.author.orcid | 0000-0002-2189-8644 | - |
crisitem.author.orcid | 0000-0001-8000-5642 | - |
crisitem.author.orcid | 0000-0001-9738-5493 | - |
crisitem.author.orcid | 0000-0002-1482-708X | - |
crisitem.author.orcid | 0000-0001-8737-255X | - |
crisitem.author.orcid | 0000-0002-1216-7831 | - |
crisitem.author.orcid | 0000-0002-6972-8388 | - |
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