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Comparative Analysis of the Spanish and Portuguese "Soft Power" Models [СРАВНИТЕЛЬНЫЙ АНАЛИЗ ИСПАНСКОЙ И ПОРТУГАЛЬСКОЙ МОДЕЛИ «МЯГКОЙ СИЛЫ»]
Borzova A., Nikolashvili N.
Optical Variability of the TeV Blazar 1ES 0806+524 on Diverse Timescales
Pandey A., Gupta A.C., Kurtanidze S.O., Wiita P.J., Damljanovic G., Bachev R., Zhang J., Kurtanidze O.M., Darriba A., Chigladze R.A., Latev G., Nikolashvili M.G., Peneva S., Semkov E., Strigachev A., Tiwari S.N., Vince O.
The historical development of the “soft power” resources of the Kingdom of Spain
Nikolashvili N.D.
EFFECT OF PROFESSIONAL BLEACHING ON THE HYGIENE OF THE ORAL CAVITY. A RANDOMIZED CONTROLLED STUDY
Vlasova N.N., Turkina A.Yu., Prokhorov N.I., Makeeva M.K., Danilina A.A., Nikolashvili N.I.
Optical and radio variability of BL Lacertae
Gaur H., Gupta A., Bachev R., Strigachev A., Semkov E., Wiita P., Volvach A., Gu M., Agarwal A., Agudo I., Aller M., Aller H., Kurtanidze O., Kurtanidze S., Lähteenmäki A., Peneva S., Nikolashvili M., Sigua L., Tornikoski M., Volvach L.
timescales and inter-band lags in these bands. Methods. We performed optical observations in B, V, R, and I
Multiwavelength temporal and spectral variability of the blazar OJ 287 during and after the 2015 December flare: A major accretion disc contribution
Hirochi J., Itoh R., Kawabata M., Kopatskaya E., Kurtanidze S., Larionova E., Larionova L., Mishra A., Morozova D., Nakaoka T., Nikolashvili M., Savchenko S., Troitskaya Y., Troitsky I., Vasilyev A.
Optical and radio variability of BL Lacertae
Gaur H., Gupta A., Bachev R., Strigachev A., Semkov E., Wiita P., Volvach A., Gu M., Agarwal A., Agudo I., Aller M., Aller H., Kurtanidze O., Kurtanidze S., Lähteenmäki A., Peneva S., Nikolashvili M., Sigua L., Tornikoski M., Volvach L.
timescales and inter-band lags in these bands. Methods. We performed optical observations in B, V, R, and I
Variability and Period Analysis for BL Lac AO 0235+164
Fan J., Kurtanidze O., Liu Y., Liu X., Yang J., Richter G., Nikolashvili M., Kurtanidze S., Wang H., Sasada M., Zhou A., Lin C., Yuan Y., Zhang Y., Costantin D.
Polarization angle swings in blazars: The case of 3C 279
Kiehlmann S., Savolainen T., Jorstad S., Sokolovsky K., Schinzel F., Marscher A., Larionov V., Agudo I., Akitaya H., Benítez E., Berdyugin A., Blinov D., Bochkarev N., Borman G., Burenkov A., Casadio C., Doroshenko V., Efimova N., Fukazawa Y., Gómez J., Grishina T., Hagen-Thorn V., Heidt J., Hiriart D., Itoh R., Joshi M., Kawabata K., Kimeridze G., Kopatskaya E., Korobtsev I., Krajci T., Kurtanidze O., Kurtanidze S., Larionova E., Larionova L., Lindfors E., López J., McHardy I., Molina S., Moritani Y., Morozova D., Nazarov S., Nikolashvili M., Nilsson K., Pulatova N., Reinthal R., Sadun A., Sasada M., Savchenko S., Sergeev S., Sigua L., Smith P., Sorcia M., Spiridonova O., Takaki K., Takalo L., Taylor B., Troitsky I., Uemura M., Ugolkova L., Ui T., Yoshida M., Zensus J., Zhdanova V.
The complex variability of blazars: Time-scales and periodicity analysis in S4 0954+65
Raiteri C.M., Villata M., Larionov V.M., Jorstad S.G., Marscher A.P., Weaver Z.R., Acosta-Pulido J.A., Agudo I., Andreeva T., Arkharov A., Bachev R., Benítez E., Berton M., Björklund I., Borman G.A., Bozhilov V., Carnerero M.I., Carosati D., Casadio C., Chen W.P., Damljanovic G., D'Ammando F., Escudero J., Fuentes A., Giroletti M., Grishina T.S., Gupta A.C., Hagen-Thorn V.A., Hart M., Hiriart D., Hou W.J., Ivanov D., Kim J.Y., Kimeridze G.N., Konstantopoulou C., Kopatskaya E.N., Kurtanidze O.M., Kurtanidze S.O., Lähteenmäki A., Larionova E.G., Larionova L.V., Marchili N., Markovic G., Minev M., Morozova D.A., Myserlis I., Nakamura M., Nikiforova A.A., Nikolashvili M.G., Otero-Santos J., Ovcharov E., Pursimo T., Rahimov I., Righini S., Sakamoto T., Savchenko S.S., Semkov E.H., Shakhovskoy D., Sigua L.A., Stojanovic M., Strigachev A., Thum C., Tornikoski M., Traianou E., Troitskaya Y.V., Troitskiy I.S., Tsai A., Valcheva A., Vasilyev A.A., Vince O., Zaharieva E.
brings significant additional information, revealing that (i) in the optical, long-term flux changes

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