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The results of 8-year R-band photopolarimetric data of blazar Mrk 421 collected from February 2008 to May 2016 are presented, along with extensive multiwavelength observations covering from radio to TeV $\gamma$-rays around the flares…

This study presents an analysis of the optical variability of the blazar 1E 1458.8+2249 on diverse timescales using multi-band observations, including observations in the optical BVRI bands carried out with the T60 and T100 telescopes from…

High Energy Astrophysical Phenomena · Physics 2024-10-25 Aykut Özdönmez , Murat Tekkeşinoğlu

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

The long-term optical and infrared color variability of blazars has been investigated with the SMARTS monitoring data. The sample in this study consists of 49 flat spectrum radio quasars and 22 BL Lac objects. The fractional variability…

Astrophysics of Galaxies · Physics 2015-11-11 Bing-Kai Zhang , Xiao-Shan Zhou , Xiao-Yun Zhao , Ben-Zhong Dai

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…

BL Lacertae (BL Lac), the archetypal blazar of its subclass and one of the most studied blazars in the last decades, has undergone a series of major multi-wavelength outbursts since 2020, resulting in its highest recorded $\gamma$-ray flare…

High Energy Astrophysical Phenomena · Physics 2026-04-08 K. Abe , S. Abe , A. Abhishek , F. Acero , A. Aguasca-Cabot , I. Agudo , C. Alispach , D. Ambrosino , F. Ambrosino , L. A. Antonelli , C. Aramo , A. Arbet-Engels , C. Arcaro , T. T. H. Arnesen , P. Aubert , A. Baktash , M. Balbo , A. Bamba , A. Baquero Larriva , U. Barres de Almeida , J. A. Barrio , L. Barrios Jiménez , I. Batkovic , J. Baxter , J. Becerra González , J. Bernete , A. Berti , E. Bissaldi , O. Blanch , G. Bonnoli , P. Bordas , A. Briscioli , G. Brunelli , J. Buces , A. Bulgarelli , I. Burelli , L. Burmistrov , M. Cardillo , S. Caroff , A. Carosi , R. Carraro , F. Cassol , D. Cerasole , A. Cerviño Cortínez , Y. Chai , G. Chon , L. Chytka , G. M. Cicciari , J. L. Contreras , J. Cortina , H. Costantini , M. Croisonnier , M. Dalchenko , G. D'Amico , P. Da Vela , F. Dazzi , A. De Angelis , M. de Bony de Lavergne , R. Del Burgo , C. Delgado , J. Delgado Mengual , D. della Volpe , B. De Lotto , L. Del Peral , R. de Menezes , G. De Palma , V. de Souza , C. Díaz , L. Di Bella , A. Di Piano , F. Di Pierro , R. Di Tria , L. Di Venere , D. Dominis Prester , A. Donini , D. Dorner , L. Eisenberger , D. Elsässer , G. Emery , L. Feligioni , F. Ferrarotto , A. Fiasson , L. Foffano , Y. Fukazawa , S. Gallozzi , R. Garcia López , S. Garcia Soto , C. Gasbarra , D. Gasparrini , J. Giesbrecht Paiva , N. Giglietto , F. Giordano , N. Godinovic , T. Gradetzke , R. Grau , J. Green , G. Grolleron , S. Gunji , P. Günther , J. Hackfeld , D. Hadasch , M. Hashizume , T. Hassan , K. Hayashi , L. Heckmann , M. Heller , J. Herrera Llorente , N. Hiroshima , D. Hoffmann , D. Horns , J. Houles , D. Hrupec , R. Imazawa , T. Inada , S. Inoue , K. Ioka , M. Iori , T. Itokawa , A. Iuliano , J. Jahanvi , I. Jimenez Martinez , J. Jimenez Quiles , I. Jorge Rodrigo , J. Jurysek , M. Kagaya , V. Karas , H. Katagiri , D. Kerszberg , T. Kiyomoto , Y. Kobayashi , K. Kohri , P. Kornecki , H. Kubo , J. Kushida , B. Lacave , M. Lainez , A. Lamastra , L. Lemoigne , M. Linhoff , S. Lombardi , F. Longo , R. López-Coto , A. López-Oramas , S. Loporchio , J. Lozano Bahilo , F. Lucarelli , H. Luciani , P. L. Luque-Escamilla , M. Makariev , M. Mallamaci , D. Mandat , K. Mannheim , F. Marini , M. Mariotti , P. Marquez , G. Marsella , J. Martí , O. Martinez , G. Martínez , M. Martínez , M. Massa , D. Mazin , J. Méndez-Gallego , S. Menon , E. Mestre Guillen , D. Miceli , T. Miener , J. M. Miranda , M. Molero Gonzalez , E. Molina , T. Montaruli , A. Moralejo , A. Morselli , V. Moya , A. L. Müller , H. Muraishi , S. Nagataki , T. Nakamori , A. Neronov , D. Nieto Castaño , M. Nievas Rosillo , L. Nikolic , K. Noda , V. Novotny , S. Nozaki , M. Ohishi , Y. Ohtani , A. Okumura , R. Orito , L. Orsini , J. Otero-Santos , P. Ottanelli , M. Palatiello , G. Panebianco , D. Paneque , R. Paoletti , J. M. Paredes , M. Pech , M. Pecimotika , M. Peresano , F. Perrotta , F. Pfeifle , M. Pihet , G. Pirola , C. Plard , F. Podobnik , M. Polo , C. Pozo-Gonzaléz , E. Prandini , S. Rainò , R. Rando , W. Rhode , M. Ribó , G. Rodriguez Fernandez , M. D. Rodríguez Frías , A. Roy , A. Ruina , E. Ruiz-Velasco , T. Saito , S. Sakurai , D. A. Sanchez , H. Sano , E. Santos Moura , T. Šarić , Y. Sato , F. G. Saturni , V. Savchenko , F. Schiavone , F. Schussler , T. Schweizer , M. Seglar Arroyo , G. Silvestri , A. Simongini , J. Sitarek , V. Sliusar , I. Sofia , J. Strišković , M. Strzys , Y. Suda , A. Sunny , H. Tajima , M. Takahashi , R. Takeishi , S. J. Tanaka , D. Tateishi , T. Tavernier , P. Temnikov , Y. Terada , K. Terauchi , T. Terzic , M. Teshima , M. Tluczykont , T. Tomura , D. F. Torres , F. Tramonti , P. Travnicek , G. Tripodo , A. Tutone , M. Vacula , M. Vázquez Acosta , G. Verna , I. Viale , A. Viana , A. Vigliano , C. F. Vigorito , E. Visentin , V. Vitale , G. Voutsinas , I. Vovk , T. Vuillaume , R. Walter , T. Yamamoto , R. Yamazaki , Y. Yao , T. Yoshida , T. Yoshikoshi , W. Zhang , N. Zywucka , the CTAO-LST collaboration , F. Aceituno , J. A. Acosta-Pulido , V. Casanova , J. Escudero Pedrosa , V. Fallah Ramazani , J. Jormanainen , S. Jorstad , G. Keating , P. M. Kouch , M. Gurwell , A. Lähteenmäki , E. Lindfors , A. Marscher , D. Morcuende , I. Myserlis , K. Nilsson , C. A. Ortega Hunter , R. Rao , A. Sota , M. Tornikoski , H. Zhang

We present the results obtained from our campaign to characterize the intra-night-optical variability properties of blazars detected by the {\it Fermi} Large Area Telescope. This involves R-band monitoring observations of a sample of 18…

High Energy Astrophysical Phenomena · Physics 2022-02-16 K. Subbu Ulaganatha Pandian , A. Natarajan , C. S. Stalin , Ashwani Pandey , S. Muneer , B. Natarajan

We present a long-term and intraday variability study on optical multiwaveband ($U\!BV\!RI$) data from the blazar AO 0235+164 collected by various telescopes for $\sim$44 years (1975--2019). The blazar was found to be significantly variable…

Blazars are the established sources of an intense and variable non-thermal radiation extending from radio wavelengths up to HE and VHE gamma-rays. Understanding the spectral evolution of blazars in selected frequency ranges, as well as…

High Energy Astrophysical Phenomena · Physics 2014-12-24 Alicja Wierzcholska , Michał Ostrowski , Łukasz Stawarz , Stefan Wagner , Marcus Hauser

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…

BL Lacertae had undergone a series of historical high flux activity over a year, from August 2020 in the optical to VHE $\gamma$-rays. In this paper, we report on optical flux and spectral variability of the first historical maxima outburst…

We present the optical (V, R, and I) photometry for BL Lacertae, which was observed from 1997 through 1999, with the 1.56-m telescope at the Shanghai astronomical observatory (SHAO). After the 1997 outburst, it dimmed to a low state and…

Astrophysics · Physics 2016-08-30 J. H. Fan , B. C. Qian , J. Tao

We present photometric observations of the BL Lacertae object S5 0716+714 with a temporal resolution of 120 s in the Sloan i' and r' bands. These observations were conducted using the Comet Search Program telescope at Xingming Observatory…

Astrophysics of Galaxies · Physics 2025-03-17 Huai-Zhen Li , Di-Fu Guo , Long-Hua Qin , Fen Liu , Hong-Tao Liu , Ting-Feng Yi , Quan-Gui Gao , Shi-Feng Huang , Xing Gao , Xu Chen

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…

New optical and radio data on the BL Lacertae object AO 0235+16 have been collected in the last four years by a wide international collaboration, which confirm the intense activity of this source. The optical data also include the results…

In this paper, we report results of our near-infrared (NIR) photometric variability studies of the BL Lacertae object S5 0716+714. NIR photometric observations spread over 7 nights during our observing run April 2-9, 2007 at 1.8 meter…

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…

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…

BL Lacertae has been the target of four observing campaigns by the Whole Earth Blazar Telescope (WEBT) collaboration. In this paper we present $UBVRI$ light curves obtained by the WEBT from 1994 to 2002, including the last, extended BL Lac…

Astrophysics · Physics 2019-08-14 M. Villata , C. M. Raiteri

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