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Related papers: Characterizing optical variability of OJ 287 in 20…

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In this contribution two papers on the BL Lac object PKS 2155-304 are presented. They are based on our program of systematic intensive optical monitoring in search of fast variability events. In the first paper the results of a CCD…

Astrophysics · Physics 2007-05-23 A. Treves , E. Pian , F. Scaltriti , E. Palazzi , L. Tommasi , E. Poretti

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

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.…

New data and results on the optical behaviour of the blazar PKS 0735+178 are presented. In addition the whole historical light curve, and a new photometric calibration of comparison stars are reported. Optical spectral indexes are…

In this work, we present the results of our multi-band microvariability study of the famous blazar BL Lac. We performed microvariablity observations of the source in the optical VRI bands for 4 nights in the year 2016. We studied the…

High Energy Astrophysical Phenomena · Physics 2017-11-27 Gopal Bhatta , James R. Webb

We present the most continuous data base of optical $BVR_{c}I_{c}$ observations ever published on the BL Lacertae object GC 0109+224, collected mainly by the robotic telescope of the Perugia University Observatory in the period November…

Astrophysics · Physics 2008-11-26 S. Ciprini , G. Tosti , C. M. Raiteri , M. Villata , M. A. Ibrahimov , G. Nucciarelli , L. Lanteri

(Abridged) OJ287 is a BL Lac object that has shown double-peaked bursts at regular intervals of ~12 yr during the last ~40 yr. We analyse optical photopolarimetric monitoring data from 2005-2009, during which the latest double-peaked…

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 selected a sample of a dozen blazars which are the prime candidates for simultaneous multi-wavelength observing campaigns in their outburst phase. We searched for optical outbursts, intra-day variability and short term variability in…

Astrophysics · Physics 2009-11-13 A. C. Gupta , J. H. Fan , J. M. Bai , S. J. Wagner

A detailed analysis of the optical polarimetric variability of the TeV blazar 1ES 1959+650 from 2007 October 18 to 2011 May 5 is presented. The source showed a maximum and minimum brightness states in the R-band of 14.08$\pm$0.03 mag and…

An analysis is presented of the optical polarimetric and multicolour photometric ($BVRJ$) behaviour of the blazar PKS 2155$-$304 during an outburst in 2010. This flare develops over roughly 117 days, with a flux doubling time $\tau \sim 11$…

High Energy Astrophysical Phenomena · Physics 2020-05-20 N. W. Peceur , A. R. Taylor , R. C. Kraan-Korteweg

A high degree of linear polarization measured in the optical emission is an important observational feature of blazars. It provides strong evidence of the presence of relativistic particles and magnetic field ordering in the non-thermal…

High Energy Astrophysical Phenomena · Physics 2025-03-17 K K Singh , A Singh , A Tolamatti , P J Meintjes , K K Yadav

We present the results of the optical monitoring of 18 southern blazars in the V and R Johnson-Cousins bands. Our main objective is to study the variations in the optical flux and theis relationship with the colour and spectral…

High Energy Astrophysical Phenomena · Physics 2024-11-26 L. Zibecchi , I. Andruchow , E. Ej. Marchesini , S. A. Cellone , J. A. Combi

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

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 report results of multiband optical monitoring of two well known blazars, S5 0716+714 and BL Lacertae, carried out in 1996 and 2000-01 with an aim to study optical variations on time scales from minutes to hours and longer.The light…

Astrophysics · Physics 2007-05-23 C. S. Stalin , Gopal-Krishna , Ram Sagar , Paul J. Wiita , V. Mohan , A. K. Pandey

We monitored the BL Lac object S5 0716+714 in the optical band during October 2008, December 2008 and February 2009 with a best temporal resolution of about 5 minutes in the BVRI bands. Four fast flares were observed with amplitudes ranging…

Astrophysics of Galaxies · Physics 2014-11-20 H. Poon , J. H. Fan , J. N. Fu

We monitored BL Lacertae frequently during 2014 - 2016 when it was generally in a high state. We searched for intra-day variability for 43 nights using quasi-simultaneous measurements in the B, V, R, and I bands (totaling 143 light curves);…

High Energy Astrophysical Phenomena · Physics 2017-12-20 Haritma Gaur , Alok C. Gupta , R. Bachev , A. Strigachev , E. Semkov , Paul J. Wiita , M. F. Gu , S. Ibryamov

We continuously monitored the blazar S5 0716+714 in the optical $g$, $r$ and $i$ bands from Nov. 10, 2017 to Jun. 06, 2019. The total number of observations is 201 nights including 26973 data points. This is a very large quasi-simultaneous…

High Energy Astrophysical Phenomena · Physics 2020-04-01 Dingrong Xiong , Jinming Bai , Junhui Fan , Dahai Yan , Minfeng Gu , Xuliang Fan , Jirong Mao , Nan Ding , Rui Xue , Weimin Yi