Weaver Z.R.; Williamson K.E.; Jorstad S.G.; Marscher A.P.; Larionov V.M.; Raiteri C.M.; Villata M.; Acosta-Pulido J.A.; Bachev R.; Baida G.V.; Balonek T.J.; Benítez E.; Borman G.A.; Bozhilov V.; Carnerero M.I.; Carosati D.; Chen W.P.; Damljanovic G.; Dhiman V.; Dougherty D.J.; Ehgamberdiev S.A.; Grishina T.S.; Gupta A.C.; Hart M.; Hiriart D.; Hsiao H.Y.; Ibryamov S.; Joner M.; Kimeridze G.N.; Kopatskaya E.N.; Kurtanidze O.M.; Kurtanidze S.O.; Larionova E.G.; Matsumoto K.; Matsumura R.; Minev M.; Mirzaqulov D.O.; Morozova D.A.; Nikiforova A.A.; Nikolashvili M.G.; Ovcharov E.; Rizzi N.; Sadun A.; Savchenko S.S.; Semkov E.; Slater J.J.; Smith K.L.; Stojanovic M.; Strigachev A.; Troitskaya Y.V.; Troitsky I.S.; Tsai A.L.; Vince O.; Valcheva A.; Vasilyev A.A.; Zaharieva E.; Zhovtan A.V.
(2020)
© 2020. The American Astronomical Society. All rights reserved.. In an effort to locate the sites of emission at different frequencies and physical processes causing variability in blazar jets, we have obtained high ...