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This report presents the results of optical polarimetric observations carried out with 6-m and 1-m telescopes at SAO RAS. The study of the blazar S5 0716+714 radiation showed the presence of a period of the variability of brightness and…

Astrophysics of Galaxies · Physics 2023-09-26 Elena Shablovinskaya , Eugene Malygin , Dmitry Oparin

In this work, we report the presence of rapid intra-night optical variations in both -- flux and polarization of the blazar BL Lacertae during its unprecedented 2020--2021 high state of brightness. The object showed significant flux…

We study the ensemble optical variability of 276 FSRQs and 86 BL Lacs in the Palomar-QUEST Survey with the goal of searching for common fluctuation properties, examining the range of behavior across the sample, and characterizing the…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-11 Anne Bauer , Charles Baltay , Paolo Coppi , Nancy Ellman , Jonathan Jerke , David Rabinowitz , Richard Scalzo

We present the results of variability power spectral density (PSD) analysis using multiwavelength radio to GeV\,$\gamma$-ray light curves covering decades/years to days/minutes timescales for the blazars 3C 279 and PKS 1510-089. The PSDs…

We present the results of the observational study of the blazar S5 0716+716 in the optical bands B, V, R, and I between March 2019 and August 2023 to investigate its variability on diverse time-scales. The blazar was followed up by the T60…

High Energy Astrophysical Phenomena · Physics 2024-07-15 Ergün Ege , Aykut Özdönmez , Aditi Agarwal , Tansel Ak

The observation data of blazar 1ES 1426 + 42.8 were obtained using the 1.02 m optical telescope of Yunnan Observatories during $2021$ to $2023$. Intraday variability (IDV) is detected on seven nights. We use the turbulent model to…

Astrophysics of Galaxies · Physics 2024-09-12 X. Chang , D. R. Xiong , T. F. Yi , C. X. Liu , G. Bhatta , J. R. Xu , Y. L. Gong

We performed a long-term optical (B, V, R bands), infra-red (J and K bands) and radio band (15, 22, 37 GHz band) study on the flat spectrum radio quasar, 3C 454.3, using the data collected over a period of more than 8 years (MJD…

We carried out a high time-resolution, multicolour optical observing campaign for eight $\gamma$-ray detected blazars during 2010-2020. We analyze flux variations, correlations between magnitudes and colours on different timescales.…

High Energy Astrophysical Phenomena · Physics 2023-02-15 X. Chang , T. F. Yi , D. R. Xiong , C. X. Liu , X. Yang , H. Z. Li , Y. L. Gong , W. W. Na , Y. Li , Z. H. Chen , J. P. Chen , L. S. Mao

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

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

(abridged) We perform photometric time-series analysis of a sample of ten early to mid-L dwarfs in the field over three years of $K_s$-band observations with the OMEGA 2000 infrared camera of the 3.5m telescope on Calar Alto Observatory…

Solar and Stellar Astrophysics · Physics 2015-06-22 Belén López Martí , María Rosa Zapatero Osorio

Blazars are a highly variable subclass of active galactic nuclei that have been observed to vary significantly during a single night. This intranight variability remains a debated phenomenon, with various mechanisms proposed to explain the…

High Energy Astrophysical Phenomena · Physics 2024-02-02 Callum McCall , Helen E. Jermak , Iain A. Steele , Shiho Kobayashi , Johan H. Knapen , Pablo M. Sánchez-Alarcón

Blazars display variable emission across the entire electromagnetic spectrum, with timescales that can range from a few minutes to several years. Our recent work has shown that a sample of five blazars exhibit hints of periodicity with a…

High Energy Astrophysical Phenomena · Physics 2023-10-20 P. Peñil , J. R. Westernacher-Schneider , M. Ajello , A. Domínguez , S. Buson , J. Otero-Santos , L. Marcotulli , N. Torres-Albà , J. Zrake

Since 1997, BL Lacertae has undergone a phase of high optical activity, with the occurrence of several prominent outbursts. Starting from 1999, the Whole Earth Blazar Telescope (WEBT) consortium has organized various multifrequency…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 M. Villata , C. M. Raiteri , V. M. Larionov , M. G. Nikolashvili , M. F. Aller

We carried out a pilot campaign of radio and optical band intra-day variability (IDV) observations of five blazars (3C66A, S5 0716+714, OJ287, B0925+504, and BL Lacertae) on December 18--21, 2015 by using the radio telescope in Effelsberg…

Temporal analysis of blazar flux is a powerful tool to draw inferences about the emission processes and physics of these sources. In the most general case, the available light curves are irregularly sampled and influenced by gaps, and in…

High Energy Astrophysical Phenomena · Physics 2020-06-10 Stefano Covino , Marco Landoni , Angela Sandrinelli , Aldo Treves

Multicolor (UBVRIJHK) observations of the blazar AO 0235+16 are analyzed. The light curves were compiled at the Turin Observatory from literature data and the results of observations obtained in the framework of the WEBT program…

Optical polarization of seven selected BL Lac objects in UBVRI bands was studied with the Nordic Optical Telescope from December 10-14, 1999. Two of them, 3C 66A and PKS 0735+178, were monitored for 4 nights for a total integration time of…

Astrophysics · Physics 2009-11-06 L. Tommasi , E. Palazzi , E. Pian , V. Piirola , E. Poretti , F. Scaltriti , A. Sillanpaa , L. Takalo , A. Treves

Characterisation of the long-term variations in the broad line region in a luminous blazar, where Comptonisation of broad-line emission within a relativistic jet is the standard scenario for production of gamma-ray emission that dominates…

High Energy Astrophysical Phenomena · Physics 2020-08-04 Krzysztof Nalewajko , Alok C. Gupta , Mai Liao , Krzysztof Hryniewicz , Maitrayee Gupta , Minfeng Gu

We monitored BL Lacertae simultaneously in the optical B, V, R and I bands for 13 nights during the period 2012-2016. The variations were well correlated in all bands and the source showed significant intraday variability (IDV). We also…

Astrophysics of Galaxies · Physics 2017-06-23 Nankun Meng , Jianghua Wu , James R. Webb , Xiaoyuan Zhang , Yan Dai
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