Multifrequency monitoring of the blazar 0716+714 during the GASP-WEBT-AGILE campaign of 2007
M. VillataNational Institute for Astrophysics, Rome, ItalyC. M. RaiteriINAF, Osservatorio Astronomico di Torino, Italy e-mail: [email protected]V. M. LarionovAstronomical Institute, St.-Petersburg State University, RussiaO. M. KurtanidzeAbastumani Astrophysical Observatory, GeorgiaK. NilssonTuorla Observatory, University of Turku, FinlandM. F. AllerDepartment of Astronomy, University of Michigan, MI, USAM. TornikoskiMetsähovi Radio Obs., Helsinki Univ. of Tech. TKK, FinlandA. E. VolvachRadio Astronomy Lab. of Crimean Astrophysical Obs., UkraineH. D. AllerDepartment of Astronomy, University of Michigan, MI, USAA. A. ArkharovPulkovo Observatory, RussiaU. BachMax-Planck-Institut für Radioastronomie, GermanyP. BeltrameGopal BhattaSARA Observatory, Florida International University, FL, USAC. S. BuemiINAF, Osservatorio Astrofisico di Catania, ItalyM. BöttcherAstrophys. Inst., Dept. of Phys. & Astron., Ohio Univ., OH, USAP. CalcideseOss. Astronomico della Regione Autonoma Valle d'Aosta, ItalyD. CarosatiArmenzano Astronomical Observatory, ItalyA. J. Castro‐TiradoInstituto de Astrofísica de Andalucía, CSIC, SpainD. Da RioA. Di PaolaINAF, Osservatorio Astronomico di Roma, ItalyM. DolciE. FornéA. FrascaINAF, Osservatorio Astrofisico di Catania, ItalyV. A. Hagen‐ThornAstronomical Institute, St.-Petersburg State University, RussiaJ. HeidtD. HiriartM. JelínekInstituto de Astrofísica de Andalucía, CSIC, SpainG. N. KimeridzeAbastumani Astrophysical Observatory, GeorgiaT. S. KonstantinovaAstronomical Institute, St.-Petersburg State University, RussiaE. N. KopatskayaAstronomical Institute, St.-Petersburg State University, RussiaL. LanteriINAF, Osservatorio Astronomico di Torino, Italy e-mail: [email protected]P. LetoINAF, Istituto di Radioastronomia Sezione di Noto, ItalyR. LigustriE. LindforsTuorla Observatory, University of Turku, FinlandA. LähteenmäkiMetsähovi Radio Obs., Helsinki Univ. of Tech. TKK, FinlandE. MarilliINAF, Osservatorio Astrofisico di Catania, ItalyE. NieppolaMetsähovi Radio Obs., Helsinki Univ. of Tech. TKK, FinlandM. G. NikolashviliAbastumani Astrophysical Observatory, GeorgiaM. PasanenTuorla Observatory, University of Turku, FinlandB. RagozzineAstrophys. Inst., Dept. of Phys. & Astron., Ohio Univ., OH, USAJ. AgramuntL. A. SiguaAbastumani Astrophysical Observatory, GeorgiaR. L. SmartINAF, Osservatorio Astronomico di Torino, Italy e-mail: [email protected]M. SorciaL. O. TakaloTuorla Observatory, University of Turku, FinlandM. TavaniINAF, IASF-Roma, ItalyC. TrigilioINAF, Osservatorio Astrofisico di Catania, ItalyR. TurchettiKyle UckertAstrophys. Inst., Dept. of Phys. & Astron., Ohio Univ., OH, USAG. UmanaINAF, Osservatorio Astrofisico di Catania, ItalyS. VercelloneINAF, IASF-Milano, ItalyJ. R. WebbSARA Observatory, Florida International University, FL, USA
2008en
ABI
Аннотация
Aims. Since the CGRO operation in 1991–2000, one of the primary unresolved questions about the blazar γ-ray emission has been its possible correlation with the low-energy (in particular optical) emission. To help answer this problem, the Whole Earth Blazar Telescope (WEBT) consortium has organized the GLAST-AGILE Support Program (GASP) to provide the optical-to-radio monitoring data to be compared with the γ-ray detections by the AGILE and GLAST satellites. This new WEBT project started in early September 2007, just before a strong γ-ray detection of 0716+714 by AGILE.
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