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Related papers: Intraday Optical Variability of BL Lacertae

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We have monitored the BL Lac object Mrk 501 in optical $V$, $R$ and $I$ bands from 2010 to 2015. For Mrk 501, the presence of strong host galaxy component can affect the results of photometry. After subtracting the host galaxy…

High Energy Astrophysical Phenomena · Physics 2016-03-23 Dingrong Xiong , Xiong Zhang , Tingfeng Yi , Jinming Bai , Fang Wang , Hongtao Liu , Yonggang Zheng , Haojing Zhang

We present an extensive recent multi-band optical photometric observations of the blazar S5 0716+714 carried out over 53 nights with two telescopes in India, two in Bulgaria, one in Serbia, and one in Egypt during 2019 November -- 2022…

Eight optical and four radio observatories have been intensively monitoring the BL Lac object 0716+714 in the last years: 4854 data points have been collected in the UBVRI bands since 1994, while radio light curves extend back to 1978. Many…

We report the flux and spectral variability of PG 1553+113 on intra-night (IDV) to short-term timescales using BVRI data collected over 91 nights from 28 February to 8 November 2019 employing ten optical telescopes: three in Bulgaria, two…

We report results based on the monitoring of the BL Lac object Mrk 501 in the optical (B, V and R) passbands from March to May 2000. Observations spread over 12 nights were carried out using 1.2 meter Mount Abu Telescope, India and 61 cm…

Astrophysics · Physics 2009-06-23 A. C. Gupta , W. G. Deng , U. C. Joshi , J. M. Bai , M. G. Lee

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

To search for optical variability on a wide range of timescales, we have carried out photometric monitoring of 3C 454.3, 3C 279 and S5 0716+714. CCD magnitudes in B, V, R and I pass-bands were determined for $\sim$ 7000 new optical…

High Energy Astrophysical Phenomena · Physics 2017-12-20 A. Agarwal , A. C. Gupta

We have monitored the flat spectrum radio quasar, 3C 279, in the optical $B$, $V$, $R$ and $I$ passbands from 2018 February to 2018 July for 24 nights, with a total of 716 frames, to study flux, colour and spectral variability on diverse…

We present the analysis results of flux and spectral variability of the blazar OP 313 across intra-night to short-term timescales using BVRI photometric data, gathered over 25 nights from Nov 2024 to May 2025, using two optical telescopes…

High Energy Astrophysical Phenomena · Physics 2025-09-11 P. U. Devanand , Alok C. Gupta , Karan Dogra , Shubham Kishore , Tushar Tripathi

Optical, near-infrared, and radio observations of the BL Lac object PKS2155-304 were obtained simultaneously with a continuous UV/EUV/X-ray monitoring campaign in 1994 May. Further optical observations were gathered throughout most of 1994.…

We report the results of optical monitoring for a sample of 11 blazars including 10 BL Lacs and 1 Flat Spectrum Radio Quasar (FSRQ). We have measured the multiband optical flux and colour variations in these blazars on intra-day and…

High Energy Astrophysical Phenomena · Physics 2013-11-21 Haritma Gaur , Alok C. Gupta , A. Strigachev , R. Bachev , E. Semkov , Paul J. Wiita , S. Peneva , S. Boeva , L. Slavcheva-Mihova , B. Mihov , G. Latev , U. S. Pandey

We have observed S5 2007+777 and 3C371 in the B and I bands for 13 and 8 nights, respectively, during various observing runs in 2001, 2002 and 2004. The observations resulted in almost evenly sampled light curves, 6-9 hours long. We do not…

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…

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 have monitored the quasar 3C 273 in optical $V$, $R$ and $I$ bands from 2005 to 2016. Intraday variability (IDV) is detected on seven nights. The variability amplitudes for most of nights are less than 10\% and four nights more than…

High Energy Astrophysical Phenomena · Physics 2017-04-05 Dingrong Xiong , Jinming Bai , Haojing Zhang , Junhui Fan , Minfeng Gu , Tingfeng Yi , Xiong Zhang

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 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…

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