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Coordinated integral and optical observations of SS433
Cherepashchuk A., Sunyaev R., Fabrikat S., Molkov S., Barsukova E., Antokhina E., Irsmambetova T., Panchenko I., Postnov K., Seifina E., Shakura N., Timokhin A., Bikmaev I., Sakhibullin N., Gnedin Y., Arkharov A., Larionov V.
by INTEGRAL together with optical spectroscopy obtained on the 6-m telescope allows us to construct a model
Coordinated integral and optical observations of SS433
Cherepashchuk A., Sunyaev R., Fabrikat S., Molkov S., Barsukova E., Antokhina E., Irsmambetova T., Panchenko I., Postnov K., Seifina E., Shakura N., Timokhin A., Bikmaev I., Sakhibullin N., Gnedin Y., Arkharov A., Larionov V.
by INTEGRAL together with optical spectroscopy obtained on the 6-m telescope allows us to construct a model
INTEGRAL observations of SS433: Results of a coordinated campaign
Cherepashchuk A., Sunyaev R., Fabrika S., Postnov K., Molkov S., Barsukova E., Antokhina E., Irsmambetova T., Panchenko I., Seifina E., Shakura N., Timokhin A., Bikmaev I., Sakhibullin N., Aslan Z., Khamitov I., Pramsky A., Sholukhova O., Gnedin Y., Arkharov A., Larionov V.
with a maximum to minimum uneclipsed hard X-ray flux ratio of ∼4 is discovered. The 18-60 keV X
INTEGRAL observations of SS433: Results of a coordinated campaign
Cherepashchuk A., Sunyaev R., Fabrika S., Postnov K., Molkov S., Barsukova E., Antokhina E., Irsmambetova T., Panchenko I., Seifina E., Shakura N., Timokhin A., Bikmaev I., Sakhibullin N., Aslan Z., Khamitov I., Pramsky A., Sholukhova O., Gnedin Y., Arkharov A., Larionov V.
with a maximum to minimum uneclipsed hard X-ray flux ratio of ∼4 is discovered. The 18-60 keV X
DISCOVERY of A HIGHLY POLARIZED OPTICAL MICROFLARE in BLAZAR S5 0716+714 during the 2014 WEBT CAMPAIGN
Bhatta G., Goyal A., Ostrowski M., Stawarz, Akitaya H., Arkharov A., Bachev R., Benítez E., Borman G., Carosati D., Cason A., Damljanovic G., Dhalla S., Frasca A., Hu S., Itoh R., Jorstad S., Jableka D., Kawabata K., Klimanov S., Kurtanidze O., Larionov V., Laurence D., Leto G., Markowitz A., Marscher A., Moody J., Moritani Y., Ohlert J., Di Paola A., Raiteri C., Rizzi N., Sadun A., Sasada M., Sergeev S., Strigachev A., Takaki K., Troitsky I., Ui T., Villata M., Vince O., Webb J., Yoshida M., Zola S., Hiriart D.
-amplitude flux variations in blazars on hourly timescales, commonly known as microvariability, is still a widely
MULTIFREQUENCY PHOTO-POLARIMETRIC WEBT OBSERVATION CAMPAIGN on the BLAZAR S5 0716+714: SOURCE MICROVARIABILITY and SEARCH for CHARACTERISTIC TIMESCALES
Bhatta G., Stawarz, Ostrowski M., Markowitz A., Akitaya H., Arkharov A., Bachev R., Benítez E., Borman G., Carosati D., Cason A., Chanishvili R., Damljanovic G., Dhalla S., Frasca A., Hiriart D., Hu S., Itoh R., Jableka D., Jorstad S., Jovanovic M., Kawabata K., Klimanov S., Kurtanidze O., Larionov V., Laurence D., Leto G., Marscher A., Moody J., Moritani Y., Ohlert J., Paola A., Raiteri C., Rizzi N., Sadun A., Sasada M., Sergeev S., Strigachev A., Takaki K., Troitsky I., Ui T., Villata M., Vince O., Webb J., Yoshida M., Zola S.
, consisting of a day-timescale modulation with superimposed hour-long microflares characterized by ∼0.1 mag
Synchrotron emission from the blazar PG 1553+113. An analysis of its flux and polarization variability
Raiteri C., Nicastro F., Stamerra A., Villata M., Larionov V., Blinov D., Acosta-Pulido J., Arévalo M., Arkharov A., Bachev R., Borman G., Carnerero M., Carosati D., Cecconi M., Chen W., Damljanovic G., Di Paola A., Ehgamberdiev S., Frasca A., Giroletti M., González-Morales P., Griñon-Marín A., Grishina T., Huang P., Ibryamov S., Klimanov S., Kopatskaya E., Kurtanidze O., Kurtanidze S., Lähteenmäki A., Larionova E., Larionova L., Lázaro C., Leto G., Liodakis I., Martínez-Lombilla C., Mihov B., Mirzaqulov D., Mokrushina A., Moody J., Morozova D., Nazarov S., Nikolashvili M., Ohlert J., Panopoulou G., Pastor Yabar A., Pinna F., Protasio C., Rizzi N., Sadun A., Savchenko S., Semkov E., Sigua L., Slavcheva-Mihova L., Strigachev A., Tornikoski M., Troitskaya Y., Troitsky I., Vasilyev A., Vera R., Vince O., Zanmar Sanchez R.
-ray variability with a time-scale of the order of 1 h. In contrast to previous results, during the brightest X
Multiwavelength behaviour of the blazar OJ 248 from radio to γ -rays
Carnerero M., Raiteri C., Villata M., Acosta-Pulido J., D'Ammando F., Smith P., Larionov V., Agudo I., Arévalo M., Arkharov A., Bach U., Bachev R., Benítez E., Blinov D., Bozhilov V., Buemi C., Bueno Bueno A., Carosati D., Casadio C., Chen W., Damljanovic G., Di Paola A., Efimova N., Ehgamberdiev S., Giroletti M., Gómez J., González-Morales P., Grinon-Marin A., Grishina T., Gurwell M., Hiriart D., Hsiao H., Ibryamov S., Jorstad S., Joshi M., Kopatskaya E., Kurtanidze O., Kurtanidze S., Lähteenmäki A., Larionova E., Larionova L., Lázaro C., Leto P., Lin C., Lin H., Manilla-Robles A., Marscher A., McHardy I., Metodieva Y., Mirzaqulov D., Mokrushina A., Molina S., Morozova D., Nikolashvili M., Orienti M., Ovcharov E., Panwar N., Pastor Yabar A., Puerto Giménez I., Ramakrishnan V., Richter G., Rossini M., Sigua L., Strigachev A., Taylor B., Tornikoski M., Trigilio C., Troitskaya Y., Troitsky I., Umana G., Valcheva A., Velasco S., Vince O., Wehrle A., Wiesemeyer H.
at the end of 2010 and beginning of 2013, revealing a complex radio-optical correlation. Crosscorrelation
DISCOVERY of A HIGHLY POLARIZED OPTICAL MICROFLARE in BLAZAR S5 0716+714 during the 2014 WEBT CAMPAIGN
Bhatta G., Goyal A., Ostrowski M., Stawarz, Akitaya H., Arkharov A., Bachev R., Benítez E., Borman G., Carosati D., Cason A., Damljanovic G., Dhalla S., Frasca A., Hu S., Itoh R., Jorstad S., Jableka D., Kawabata K., Klimanov S., Kurtanidze O., Larionov V., Laurence D., Leto G., Markowitz A., Marscher A., Moody J., Moritani Y., Ohlert J., Di Paola A., Raiteri C., Rizzi N., Sadun A., Sasada M., Sergeev S., Strigachev A., Takaki K., Troitsky I., Ui T., Villata M., Vince O., Webb J., Yoshida M., Zola S., Hiriart D.
-amplitude flux variations in blazars on hourly timescales, commonly known as microvariability, is still a widely
The beamed jet and quasar core of the distant blazar 4C 71.07
Raiteri C., Villata M., Carnerero M., Acosta-Pulido J., Mirzaqulov D., Larionov V., Romano P., Vercellone S., Agudo I., Arkharov A., Bach U., Bachev R., Baitieri S., Borman G., Boschin W., Bozhilov V., Butuzova M., Calcidese P., Carosati D., Casadio C., Chen W., Damljanovic G., Di Paola A., Doroshenko V., Efimova N., Ehgamberdiev S., Giroletti M., Gómez J., Grishina T., Ibryamov S., Jermak H., Jorstad S., Kimeridze G., Klimanov S., Kopatskaya E., Kurtanidze O., Kurtanidze S., Lähteenmäki A., Larionova E., Marscher A., Mihov B., Minev M., Molina S., Moody J., Morozova D., Nazarov S., Nikiforova A., Nikolashvili M., Ovcharov E., Peneva S., Righini S., Rizzi N., Sadun A., Samal M., Savchenko S., Semkov E., Sigua L., Slavcheva-Mihova L., Steele I., Strigachev A., Tornikoski M., Troitskaya Y., Troitsky I., Vince O.
© 2019 The Author(s). The object 4C 71.07 is a high-redshift blazar whose spectral energy

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