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The Bright γ-ray Flare of 3C 279 in 2015 June: AGILE Detection and Multifrequency Follow-up Observations
Chen W., Ehgamberdiev S., Goded A., Grishina T., Hiriart D., Hsiao H., Jorstad S., Kimeridze G., Kopatskaya E., Kurtanidze O., Kurtanidze S., Larionov V., Larionova L., Marscher A., Mirzaqulov D., Morozova D., Nilsson K., Samal M., Sigua L., Spassov B., Strigachev A., Takalo L., Antonelli L., Bulgarelli A., Cattaneo P., Colafrancesco S., Giommi P., Longo F., Morselli A., Paoletti F.
and the results of the multifrequency follow-up observations of a bright γ-ray flare of the blazar 3C 279 in 2015
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
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
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 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.
from a few hours to a few days. However, these are not persistent, as they differ in the various TESS
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
Multiwavelength Variability of BL Lacertae Measured with High Time Resolution
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.
obtained high time-resolution observations of BL Lacertae over a wide wavelength range: with the Transiting
Stochastic Modeling of Multiwavelength Variability of the Classical BL Lac Object OJ 287 on Timescales Ranging from Decades to Hours
Goyal A., Stawarz, Zola S., Marchenko V., Soida M., Nilsson K., Ciprini S., Baran A., Ostrowski M., Wiita P., Gopal-Krishna, Siemiginowska A., Sobolewska M., Jorstad S., Marscher A., Aller M., Aller H., Hovatta T., Caton D., Reichart D., Matsumoto K., Sadakane K., Gazeas K., Kidger M., Piirola V., Jermak H., Alicavus F., Baliyan K., Baransky A., Berdyugin A., Blay P., Boumis P., Boyd D., Bufan Y., Torrent M., Campos F., Gómez J., Dalessio J., Debski B., Dimitrov D., Drozdz M., Er H., Erdem A., Pérez A., Ramazani V., Filippenko A., Gafton E., Garcia F., Godunova V., Pinilla F., Gopinathan M., Haislip J., Haque S., Harmanen J., Hudec R., Hurst G., Ivarsen K., Joshi A., Kagitani M., Karaman N., Karjalainen R., Kaur N., Kozieł-Wierzbowska D., Kuligowska E., Kundera T., Kurowski S., Kvammen A., Lacluyze A., Lee B., Liakos A., Haro J., Moore J., Mugrauer M., Nogues R., Neely A., Ogloza W., Okano S., Pajdosz U., Pandey J., Perri M., Poyner G., Provencal J., Pursimo T., Raj A., Rajkumar B., Reinthal R., Reynolds T., Saario J., Sadegi S.
to construct for the first time the optical variability power spectrum of a blazar without any gaps across ∼6

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