Results of WEBT, VLBA and RXTE monitoring of 3C 279 during 2006–2007
V. M. LarionovAstron. Inst., St.-Petersburg State Univ., Russia e-mail: [email protected]S. G. JorstadAstron. Inst., St.-Petersburg State Univ., Russia e-mail: [email protected]Alan P. MarscherInst. for Astrophys. Research, Boston Univ., MA, USAC. M. RaiteriINAF, Osservatorio Astronomico di Torino, ItalyM. VillataINAF, Osservatorio Astronomico di Torino, ItalyI. AgudoInstituto de Astrofísica de Andalucía, CSIC, Granada, SpainM. F. AllerDepartment of Astronomy, University of Michigan, MI, USAA. A. ArkharovPulkovo Observatory, St.-Petersburg, RussiaI. M. AsfandiyarovUlugh Beg Astron. Inst., Tashkent, UzbekistanU. BachMax-Planck-Institut für Radioastronomie, Bonn, GermanyR. BachevInst. of Astron., Bulgarian Acad. of Sciences, Sofia, BulgariaA. BerdyuginTuorla Observatory, Univ. of Turku, Piikkiö, FinlandMarkus BöttcherDepartment of Physics and Astronomy, Ohio Univ., OH, USAC. S. BuemiINAF, Osservatorio Astrofisico di Catania, ItalyP. CalcideseOss. Astronomico della Regione Autonoma Valle d'Aosta, ItalyD. CarosatiArmenzano Astronomical Observatory, ItalyP. CharlotLab. d'Astrophys., Univ. Bordeaux 1, CNRS, Floirac, FranceW-P ChenInstitute of Astronomy, National Central University, TaiwanA. Di PaolaINAF, Osservatorio Astronomico di Roma, ItalyM. DolciINAF, Osservatorio Astronomico di Collurania Teramo, ItalyS.S. DoğruCOMU Observatory, TurkeyVictor DoroshenkoCrimean Astrophysical Observatory, UkraineYu. S. EfimovCrimean Astrophysical Observatory, UkraineA. ErdemCOMU Observatory, TurkeyA. FrascaINAF, Osservatorio Astrofisico di Catania, ItalyL. FuhrmannMax-Planck-Institut für Radioastronomie, Bonn, GermanyP. GiommiL. GlowienkaDepartment of Phys. and Astron. Univ. of Aarhus, DenmarkA. C. GuptaARIES, Manora Peak, Nainital, IndiaMark GurwellHarvard-Smithsonian Center for Astroph., Cambridge, MA, USAV. A. Hagen‐ThornAstron. Inst., St.-Petersburg State Univ., Russia e-mail: [email protected]W.‐S. HsiaoInstitute of Astronomy, National Central University, TaiwanM. IbrahimovUlugh Beg Astron. Inst., Tashkent, UzbekistanB. JordanMoscow Univ., Crimean Lab. of Sternberg Astron. Inst., UkraineM. KamadaAstronomical Institute, Osaka Kyoiku University, JapanT. S. KonstantinovaAstron. Inst., St.-Petersburg State Univ., Russia e-mail: [email protected]E. N. KopatskayaAstron. Inst., St.-Petersburg State Univ., Russia e-mail: [email protected]Y. Y. KovalevAstro Space Centre of Lebedev Physical Inst., Moscow, RussiaYu. A. KovalevAstro Space Centre of Lebedev Physical Inst., Moscow, RussiaO. M. KurtanidzeAbastumani Astrophysical Observatory, GeorgiaA. LähteenmäkiMetsähovi Radio Obs., Helsinki Univ. of Technology, FinlandL. LanteriINAF, Osservatorio Astronomico di Torino, ItalyL. V. LarionovaAstron. Inst., St.-Petersburg State Univ., Russia e-mail: [email protected]P. LetoINAF, Istituto di Radioastronomia, Sezione di Noto, ItalyP. CampionLab. d'Astrophys., Univ. Bordeaux 1, CNRS, Floirac, FranceChung‐Uk LeeKorea Astronomy and Space Science Institute, South KoreaE. LindforsTuorla Observatory, Univ. of Turku, Piikkiö, FinlandE. MarilliINAF, Osservatorio Astrofisico di Catania, ItalyI. McHardyUniversity of Southampton, UKМ. Г. МингалиевSpecial Astrophysical Observatory, N. Arkhyz, RussiaS. V. NazarovCrimean Astrophysical Observatory, UkraineE. NieppolaMetsähovi Radio Obs., Helsinki Univ. of Technology, FinlandK. NilssonTuorla Observatory, Univ. of Turku, Piikkiö, FinlandJ. OhlertM. PasanenTuorla Observatory, Univ. of Turku, Piikkiö, FinlandD. PorterCardiff University, Wales, UKT. PursimoNordic Optical Telescope, Santa Cruz de La Palma, SpainJ. AgramuntKunihiko SadakaneAstronomical Institute, Osaka Kyoiku University, JapanA. C. SadunDept. of Phys., Univ. of Colorado, Denver, USAС. Г. СергеевCrimean Astrophysical Observatory, UkraineN. SmithCork Institute of Technology, Cork, IrelandA. StrigachevInst. of Astron., Bulgarian Acad. of Sciences, Sofia, BulgariaN. SumitomoAstronomical Institute, Osaka Kyoiku University, JapanL. O. TakaloTuorla Observatory, Univ. of Turku, Piikkiö, FinlandK. TanakaAstronomical Institute, Osaka Kyoiku University, JapanC. TrigilioINAF, Osservatorio Astrofisico di Catania, ItalyG. UmanaINAF, Osservatorio Astrofisico di Catania, ItalyH. UngerechtsInstituto de Radioastronomía Milimétrica, Granada, SpainA. E. VolvachRadio Astron. Lab. of Crimean Astroph. Observatory, UkraineWu YuanYNAO, Chinese Academy of Sciences, Kunming, PR China
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Аннотация
Context. The quasar 3C 279 is among the most extreme blazars in terms of luminosity and variability of flux at all wavebands. Its variations in flux and polarization are quite complex and therefore require intensive monitoring observations at multiple wavebands to characterise and interpret the observed changes.
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