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Related papers: Longterm Optical Monitoring of Bright BL Lacertae …

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Blazars are beamed active galactic nuclei known for their strong multi-wavelength variability on timescales from years down to minutes. We aim to investigate the suitability of the twisting jet model presented in previous works to explain…

High Energy Astrophysical Phenomena · Physics 2024-12-03 C. M. Raiteri , M. Villata , M. I. Carnerero , S. O. Kurtanidze , D. O. Mirzaqulov , E. Benítez , G. Bonnoli , D. Carosati , J. A. Acosta-Pulido , I. Agudo , T. S. Andreeva , G. Apolonio , R. Bachev , G. A. Borman , V. Bozhilov , L. F. Brown , W. Carbonell , C. Casadio , W. P. Chen , G. Damljanovic , S. A. Ehgamberdiev , D. Elsaesser , J. Escudero , M. Feige , A. Fuentes , D. Gabellini , K. Gazeas , M. Giroletti , T. S. Grishina , A. C. Gupta , M. A. Gurwell , V. A. Hagen-Thorn , G. M. Hamed , D. Hiriart , M. Hodges , R. Z. ivanidze , D. V. Ivanov , M. D. Joner , S. G. Jorstad , M. D. Jovanovic , S. Kiehlmann , G. N. Kimeridze , E. N. Kopatskaya , Yu. A. Kovalev , Y. Y. Kovalev , O. M. Kurtanidze , A. Kurtenkov , E. G. Larionova , A. Lessing , H. C. Lin , J. M. López , C. Lorey , J. Ludwig , N. Marchili , A. Marchini , A. P. Marscher , K. Matsumoto , W. Max-Moerbeck , B. Mihov , M. Minev , M. G. Mingaliev , A. Modaressi , D. A. Morozova , F. Mortari , T. V. Mufakharov , I. Myserlis , M. G. Nikolashvili , T. J. Pearson , A. V. Popkov , I. A. Rahimov , A. C. S. Readhead , D. Reinhart , R. Reeves , S. Righini , F. D. Romanov , S. S. Savchenko , E. Semkov , E. V. Shishkina , L. A. Sigua , L. Slavcheva-Mihova , Yu. V. Sotnikova , R. Steineke , M. Stojanovic , A. Strigachev , A. Takey , E. Traianou , Yu. V. Troitskaya , I. S. Troitskiy , A. L. Tsai , A. Valcheva , A. A. Vasilyev , G. Verna , O. Vince , K. Vrontaki , Z. R. Weaver , J. Webb , Q. X. Yuldoshev , E. Zaharieva , A. V. Zhovtan

We report on long-term multi-wavelength monitoring of blazar Mrk 421 by the GASP-WEBT collaboration and Steward Observatory, and by the Swift and Fermi satellites. We study the source behaviour in the period 2007-2015, characterized by…

High Energy Astrophysical Phenomena · Physics 2019-08-14 M. I. Carnerero , C. M. Raiteri , M. Villata , J. A. Acosta-Pulido , V. M. Larionov , P. S. Smith , F. D'Ammando

We monitored BL Lacertae for 13 nights in optical B, V, R, and I bands during October and November 2014 including quasi-simultaneous observations in V and R bands using two optical telescopes in India. We have studied multi-band optical…

Astrophysics of Galaxies · Physics 2015-06-02 Aditi Agarwal , Alok C. Gupta

Aims. We use a sample of 83 core-dominated active galactic nuclei (AGN) selected from the MOJAVE (Monitoring of Jets in AGN with VLBA Experiments) radio-flux-limited sample and detected with the Fermi Large Area Telescope (LAT) to study the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 T. G. Arshakian , J. León-Tavares , M. Boettcher , J. Torrealba , V. H. Chavushyan , M. L. Lister , E. Ros , J. A. Zensus

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

Our recent progress on time-dependent modeling of the multiwavelength spectra and variability of blazars with leptonic and hadronic jet models is reviewed. Special emphasis is placed on X-ray spectral variability of low-frequency peaked…

Astrophysics · Physics 2007-05-23 M. Boettcher

Due to its peculiar and highly variable nature, the blazar 3C 454.3 has been extensively monitored by the WEBT team. Here, we present for the first time these long-term optical flux and color variability results using data acquired in B, V,…

Blazars optical emission is generally dominated by relativistic jets, although the host galaxy, accretion disk and broad line region (BLR) may also contribute significantly. Disentangling their contributions has been challenging for years…

We collect the 2LAC and MOJAVE quasi-simultaneous data to investigate the radio-gamma connection of blazars. The cross sample contains 166 sources. The statistic analysis based on this sample confirms positive correlations between these two…

High Energy Astrophysical Phenomena · Physics 2014-09-03 Fan Xu-Liang , Bai Jin-Ming , Liu Hong-Tao , Chen Liang , Liao Neng-Hui

We present the results of a series of radio, optical, X-ray and gamma-ray observations of the BL Lac object S50716+714 carried out between April 2007 and January 2011. The multi-frequency observations were obtained using several ground and…

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

Radio-bright BL Lacertae objects (BLOs) are typically variable and exhibit prominent flaring. We use a sample of 24 BLOs to get a clear idea of their flaring behavior and to find possible commonalities in their variability patterns. Our…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 E. Nieppola , T. Hovatta , M. Tornikoski , E. Valtaoja , M. F. Aller , H. D. Aller

Context. We present the light curves of six BL Lac objects, PKS 0537-441, PKS 0735+17, OJ 287, PKS 2005-489, PKS 2155-304, W Comae, and of the flat spectrum radio quasar PKS 1510-089, as a part of a photometric monitoring program in the…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Angela Sandrinelli , Stefano Covino , Aldo Treves

We present a polarization variability analysis of a sample of 26 $\gamma$-ray blazars monitored by the Steward Observatory between 2008 and 2018 in the optical band. We investigate the properties and long-term variability of their optical…

BL Lacertae objects are an extreme subclass of AGNs showing rapid and large-amplitude variability, high and variable polarization, and core-dominated radio emissions. If a strong beaming effect is the cause of the extreme observation…

Astrophysics · Physics 2007-05-23 J. H. Fan , K. S. Cheng , L. Zhang

Blazars are powerful, variable emitters from radio to gamma-ray wavelengths. Even though the general picture of synchrotron emission at low energies and inverse Compton at the high energy end is well established, many important aspects of…

High Energy Astrophysical Phenomena · Physics 2019-08-15 W. Max-Moerbeck , J. L. Richards , V. Pavlidou , T. J. Pearson , A. C. S. Readhead , T. Hovatta , O. G. King , R. Reeves

Decade-long monitoring of blazars at optical and infrared (OIR) wavelengths with the Small and Moderate Aperture Research Telescope System (SMARTS) in Chile and in $\gamma$-rays with the Fermi Large Area Telescope (LAT) has enabled the…

High Energy Astrophysical Phenomena · Physics 2021-07-14 M. Polkas , M. Petropoulou , G. Vasilopoulos , A. Mastichiadis , M. C. Urry , P. Coppi , C. Bailyn

BL Lac objects are active nuclei, hosted in massive elliptical galaxies, the emission of which is dominated by a relativistic jet closely aligned with the line of sight. This implies the existence of a parent population of sources with a…

High Energy Astrophysical Phenomena · Physics 2016-11-26 Renato Falomo , Elena Pian , Aldo Treves

Among active galactic nuclei, blazars show extreme variability properties. We here investigate the case of the BL Lac object S4 0954+65 with data acquired in 2019-2020 by the Transiting Exoplanet Survey Satellite (TESS) and by the Whole…

High Energy Astrophysical Phenomena · Physics 2021-05-12 C. M. Raiteri , M. Villata , V. M. Larionov , S. G. Jorstad , A. P. Marscher , Z. R. Weaver

Blazars, the peculiar class of active galactic nuclei (AGN), are known to show flux variations across the accessible electromagnetic spectrum. Though they have been studied extensively for their flux variability characteristics across…

High Energy Astrophysical Phenomena · Physics 2024-08-13 M. Reshma , Aditi Agarwal , C. S. Stalin , Prajwel Joseph , Akanksha Dagore , Amit Kumar Mandal , Ashish Devaraj , S. B. Gudennavar