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Related papers: Variability and spectral variation of 3C 66A

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We report the main results of our six year long intensive optical monitoring on blazars ON 231 (W Com), BL Lac, and 3C 273. Intensive optical monitoring is an indispensable tool to obtain well sampled light curves and thus to understand the…

Astrophysics · Physics 2010-12-13 G. Tosti , S. Ciprini , E. Massaro , M. Maesano , F. Montagni , R. Nesci

A huge multiwavelength campaign targeting the blazar AO 0235+164 was organized by the Whole Earth Blazar Telescope (WEBT) in 2003-2005 to study the variability properties of the source. Monitoring observations were carried out at cm and mm…

Astrophysics · Physics 2009-11-11 C. M. Raiteri , M. Villata , M. Kadler , M. A. Ibrahimov , O. M. Kurtanidze , V. M. Larionov

We present the analysis and results of recent high-energy gamma-ray observations of the BL Lac object 3C 66A conducted with the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE). During the 2003-2004 observing season, STACEE…

We present our photometric monitoring of a flat spectrum radio quasar (FSRQ) 3C 454.3 at Yunnan observatories from 2006 to 2011. We find that the optical color of 3C 454.3 shows obvious redder-when-brighter trend, which reaches a saturation…

High Energy Astrophysical Phenomena · Physics 2018-04-11 Xu-Liang Fan , Shao-Kun Li , Neng-Hui Liao , Liang Chen , Hong-Tao Liu , Kai-Xing Lu , Da-Hai Yan , Rui-Yu Zhang , Qian Guo , Qingwen Wu , Jin-Ming Bai

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

The quasar-type blazar 4C 38.41 (B3 1633+382) experienced a large outburst in 2011, which was detected throughout the entire electromagnetic spectrum. We present the results of low-energy multifrequency monitoring by the GASP project of the…

We have observed S4 0954+658 in the BVRI bands in 2001, and in the BI bands in 2002. The observations resulted in almost evenly sampled light curves, 3-8 hours long, with an average sampling interval of ~5-15 min. Because of the dense…

Astrophysics · Physics 2009-11-10 I. E. Papadakis , V. Samaritakis , P. Boumis , J. Papamastorakis

We report on quasi-periodic variability found in two blazars included in the Steward Observatory Blazar Monitoring data sample: the BL Lac object 3C 66A and the Flat Spectrum Radio Quasar B2 1633+38. We collect optical photometric and…

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…

BL Lac has entered an active state since 2020, with multiwavelength observations revealing intense flares. In this study, we conducted 12-night multicolor optical monitoring using an 85 cm telescope from 2020 September to 2024 June and…

High Energy Astrophysical Phenomena · Physics 2026-03-05 Hanxiao Xia , Ziming Wang , Jianghua Wu , Yue Fang , Shiyu Du

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…

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

We monitored the flaring blazar 3C 454.3 during 2005 June-July with the Spitzer Infrared Spectrograph (IRS: 15 epochs), Infrared Array Camera (IRAC: 12 epochs) and Multiband Imaging Photometer (MIPS: 2 epochs). We also made Spitzer IRS,…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Patrick M. Ogle , Ann E. Wehrle , Thomas Balonek , Mark A. Gurwell

We monitored BL Lacertae in the B, V, R and I bands for 14 nights during the period of 2016-2018. The source showed significant intraday variability on 12 nights. We performed colour-magnitude analysis and found that the source exhibited…

Astrophysics of Galaxies · Physics 2021-12-08 Tian Li , Jianghua Wu , Nankun Meng , Yan Dai , Xiaoyuan Zhang

During 1995, the broad-line radio galaxy 3C 390.3 is the subject of a multi-wavelength monitoring campaign comprised of ROSAT HRI, IUE, and ground based optical, infrared and radio observations. We report preliminary results from the…

We present the results of the blazar 3C 345 monitoring in Johnson-Cousins BVRI bands for the period 1996 - 2006. We have collected 29 V and 43 R data points for this period; the BI light curves contain a few measurements only. The accuracy…

Astrophysics · Physics 2009-11-13 B. Mihov , R. Bachev , L. Slavcheva-Mihova , A. Strigachev , E. Semkov , G. Petrov

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…

We present the observational results of multi-colour optical monitoring of eight red blazars from 2003 September to 2004 February. The aim of our monitoring is to investigate the spectral variability as well as the flux variations at short…

Astrophysics · Physics 2009-11-11 Minfeng Gu , C. -U. Lee , Soojong Pak , H. S. Yim , A. B. Fletcher

We reported the result of long term optical variability of the blazar 4C 29.45 (QSO 1156+295, Ton 599), carried out optical photometric observations in Johnson V, Cousins RI passbands during April 1997 to March 2002 using the 1.56 meter…

Astrophysics · Physics 2015-06-24 J. H. Fan , J. Tao , B. C. Qian , A. C. Gupta , Y. Liu , Y. H. Yuan , J. H. Yang , H. G. Wang , Y. Huang

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