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We have monitored the BL Lac object S5 0716+714 in five intermediate optical wavebands from 2004 September to 2011 April. Here we present the data that include 8661 measurements which represents one of the largest databases obtained for an…

High Energy Astrophysical Phenomena · Physics 2015-06-12 Yan Dai , Jianghua Wu , Zong-Hong Zhu , Xu Zhou , Jun Ma , Qirong Yuan , Lingzhi Wang

We present a multi-frequency, dense radio monitoring program of the blazar OJ287 using the 100m Effelsberg radio telescope. We analyze the evolution in total flux density, linear and circular polarization to study the jet structure and its…

High Energy Astrophysical Phenomena · Physics 2018-11-14 I. Myserlis , S. Komossa , E. Angelakis , J. L. Gómez , V. Karamanavis , T. P. Krichbaum , U. Bach , D. Grupe

We present long term optical and near infrared flux variability analysis of 37 blazars detected in the $\gamma$-ray band by the {\it Fermi Gamma-Ray Space Telescope}. Among them, 30 are flat spectrum radio quasars (FSRQs) and 7 are BL Lac…

High Energy Astrophysical Phenomena · Physics 2020-08-28 P. Z. Safna , C. S. Stalin , Suvendu Rakshit , Blesson Mathew

We present the results of extensive multi-band intra-night optical monitoring of BL Lacertae during 2010--2012. BL Lacertae was very active in this period and showed intense variability in almost all wavelengths. We extensively observed it…

Variability amplitudes larger than 1 magnitude over time-scales of a few tens of minutes have recently been reported in the optical light-curves of several blazars. In order to independently verify the real occurrence of such extremely…

Astrophysics · Physics 2008-11-26 Sergio A. Cellone , Gustavo E. Romero , Anabella T. Araudo

We present the result of near-infrared and optical observations of the BL Lac object S5 0716$ + $714 carried out by the KANATA telescope. S5 0716$ + $714 has both a long term high-amplitude variability and a short-term variability within a…

We present the results of a broadband radio-to-GeV observing campaign organized to get a better understanding of the radiation processes responsible for the $\gamma$-ray flares observed in 3C 279. The total intensity and polarization…

High Energy Astrophysical Phenomena · Physics 2016-10-26 B. Rani , T. P. Krichbaum , S. -S. Lee , K. Sokolovsky , S. Kang , D. -Y. Byun , D. Mosunova , J. A. Zensus

We carried out multi-color optical monitoring of a sample of ten blazars from 2005 to 2011. The sample contains 3 LBLs, 2 IBLs, 4 HBLs, and 1 FSRQ. Our monitoring focused on the long-term variability and the sample included nine BL Lac…

Astrophysics of Galaxies · Physics 2018-08-08 Nankun Meng , Xiaoyuan Zhang , Jianghua Wu , Jun Ma , Xu Zhou

The latest flare of the regular $\sim$ 12 years quasi-periodic optical outbursts in the binary SMBH candidate system OJ 287 occurred in December 2015. Following this, the source has exhibited enhanced multi-wavelength (MW) variability in…

High Energy Astrophysical Phenomena · Physics 2023-06-07 Pankaj Kushwaha , E. M. de Gouveia Dal Pino , Alok C. Gupta , Paul J. Wiita

This paper aims to study the color behavior of the BL Lac object OJ 287 during optical outburst. According to the revisit of the data from the OJ-94 monitoring project and the analysis the data obtained with the 60/90 cm Schmidt Telescope…

Astrophysics of Galaxies · Physics 2015-05-20 Yan Dai , Jianghua Wu , Zong-Hong Zhu , Xu Zhou , Jun Ma

We have obtained simultaneous and continuous photo-polarization observations of the blazar BL Lacertae in optical and near-infrared (NIR) bands during a historical outburst from 2020 to 2021. In total, fourteen nights of observations were…

We report the first extensive optical flux and spectral variability study of the TeV blazar TXS 0506+056 on intra-night to long-term timescales using BVRI data collected over 220 nights between January 21, 2017 to April 9, 2022 using 8…

Light curves for more than century optical photometric observations of the blazar OJ 287 reveals strong flares with a quasi-period of about 12 years. For a long time, this period has been interpreted by processes in a binary black hole…

High Energy Astrophysical Phenomena · Physics 2021-03-26 M. S. Butuzova , A. B. Pushkarev

The blazar 3C454.3 exhibited a strong flare seen in gamma-rays, X-rays, and optical/NIR bands during 3--12 December 2009. Emission in the V and J bands rose more gradually than did the gamma-rays and soft X-rays, though all peaked at nearly…

Multiband optical photometry data of blazar S5 0716+714 obtained from 2002 to 2019 reveal stable color index change with flux variability. We analyzed this trend under variability caused by the Doppler factor change in the presence of a…

High Energy Astrophysical Phenomena · Physics 2022-04-05 Mark A. Gorbachev , Marina S. Butuzova , Sergey G. Sergeev , Sergey V. Nazarov , Alexey V. Zhovtan

We present the results of photometric observations of three TeV blazars, 3C 66A, S5 0954+658 and BL Lacertae, during the period 2013--2017. Our extensive observations were performed in a total of 360 nights which produced $\sim$6820 image…

Blazars show optical and $\gamma$-ray flux variations that are generally correlated, although there are exceptions. Here we present anomalous behaviour seen in the blazar 3C 454.3 based on an analysis of quasi-simultaneous data at optical,…

High Energy Astrophysical Phenomena · Physics 2019-04-10 Bhoomika Rajput , C. S. Stalin , S. Sahayanathan , Suvendu Rakshit , Amit Kumar Mandal

We present a comprehensive analysis of the time-resolved spectral energy distributions (SEDs) of the blazar OJ 287 over a 15-year period (2008-2023), using multi-wavelength data. In the $\gamma$-ray band, multiple flaring episodes were…

High Energy Astrophysical Phenomena · Physics 2025-04-30 G. Harutyunyan , N. Sahakyan , D. Bégué

We report the study of a huge optical intraday flare on November 12, 2021, at 2 am UT, in the blazar OJ287. In the binary black hole model it is associated with an impact of the secondary black hole on the accretion disk of the primary. Our…

We present the results of multiband observations of the blazar S5 0716+714 intra-night variability performed during 23 nights in the period from 04.2014 through 04.2015. The bluer-when-brighter trend is detected in both intra- and…

Astrophysics of Galaxies · Physics 2021-03-17 Marina S. Butuzova