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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

Blazars are characterized by rapid variability at virtually all wavelengths from radio through TeV gamma-rays. The challenge since their discovery has been to understand the origin of their luminous, apparently nonthermal, nuclear emission.…

Astrophysics · Physics 2007-05-23 C. Megan Urry

The parsec-scale radio properties of 232 active galactic nuclei (AGNs), most of which are blazars, detected by the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope have been observed contemporaneously by the Very Long…

High Energy Astrophysical Phenomena · Physics 2015-06-11 J. D. Linford , G. B. Taylor , F. K. Schinzel

We examine the 2008-2016 gamma-ray and optical light curves of a number of bright Fermi blazars. In a fraction of them, the periodograms show possible evidence of quasi-periodicities related in the two bands. This coincidence strengthens…

High Energy Astrophysical Phenomena · Physics 2017-06-28 Stefano Covino , Angela Sandrinelli , Aldo Treves

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

During the last 40-50 years, the TeV blazar Ton 599 has systematically experienced major outbursts detected in a wide wavelength range from radio to $\gamma$-rays. In this work, we present an analysis of Ton 599 quasi-periodic variability…

The production site and process responsible for the highly variable high-energy emission observed from blazar jets are still debated. Gravitational lenses can be used as microscopes to investigate the nature of such sources. We study the…

High Energy Astrophysical Phenomena · Physics 2025-10-09 Sarah M. Wagner , Jeffrey D. Scargle , Greg Madejski , Andrea Gokus , Krzysztof Nalewajko , Patrick Günther , Karl Mannheim

We study the ensemble optical variability of 276 FSRQs and 86 BL Lacs in the Palomar-QUEST Survey with the goal of searching for common fluctuation properties, examining the range of behavior across the sample, and characterizing the…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-11 Anne Bauer , Charles Baltay , Paolo Coppi , Nancy Ellman , Jonathan Jerke , David Rabinowitz , Richard Scalzo

We present results from the first dedicated study in the time domain of the hard X-ray variability behavior of blazars on long timescales based on $\sim$13 years of continuous hard X-ray data in the 14-195 keV band. We use monthly-binned…

High Energy Astrophysical Phenomena · Physics 2023-10-10 Sergio Mundo , Richard Mushotzky

Blazars are jet-dominated extragalactic objects characterized by the emission of strongly variable non-thermal radiation across the entire electromagnetic spectrum. Therefore, the study of blazars (and in general of radio loud AGN) through…

High Energy Astrophysical Phenomena · Physics 2019-08-15 C. Monte , S. Raino , F. Gargano , S. Cutini , D. Gasparrini , J. Leon Tavares , G. Polenta

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 search for the long-term variability of the \gamma-ray sky in the energy range E > 1 GeV with 168 weeks of Fermi-LAT data. We perform a full sky blind search for regions with variable flux looking for deviations from uniformity. We bin…

High Energy Astrophysical Phenomena · Physics 2015-06-03 M. S. Pshirkov , G. I. Rubtsov

The LAT instrument, onboard the Fermi satellite, in its first three months of operation detected more than 100 blazars at more than the 10 sigma level. This is already a great improvement with respect to its predecessor, the instrument…

Cosmology and Nongalactic Astrophysics · Physics 2009-12-18 G. Ghisellini

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…

The blazar 3C 454.3 was revealed by the Fermi Gamma-ray Space Telescope to be in an exceptionally high flux state in July 2008. Accordingly, we performed a multi-wavelength monitoring campaign on this blazar using IR and optical…

Astrophysics · Physics 2011-02-11 E. W. Bonning , C. Bailyn , C. M. Urry , M. Buxton , G. Fossati , L. Maraschi , P. Coppi , R. Scalzo , J. Isler , A. Kaptur

Blazars are an extreme subclass of active galactic nuclei. Their rapid variability, luminous brightness, superluminal motion, and high and variable polarization are probably due to a beaming effect. However, this beaming factor (or Doppler…

High Energy Astrophysical Phenomena · Physics 2017-02-21 J. H. Fan , J. H. Yang , H. B. Xiao , C. Lin , D. Constantin , G. Y. Luo , Z. Y. Pei , J. M. Hao , Y. W. Mao

In this work, I have presented a multi-frequency variability and correlation study of the blazar Ton 599, which was observed first time in flaring state at the end of 2017. Data from \textit{Fermi}-LAT, Swift-XRT/UVOT, Steward Observatory,…

High Energy Astrophysical Phenomena · Physics 2019-01-30 Raj Prince

The advent of Fermi is changing our understanding on the radio and gamma-ray emission in Active Galactic Nuclei. In fact, contrary to previous campaigns, Fermi mission reveals that BL Lac objects are the most abundant emitters in gamma-ray…

High Energy Astrophysical Phenomena · Physics 2013-06-05 E. Liuzzo , B. Boccardi , M. Giroletti , G. Giovannini

Radio emission in blazars -- the aligned subset of Active Galactic Nuclei (AGN) -- is produced by synchrotron electrons moving relativistically in their jet's magnetic field. Under the assumption of some degree of uniformity of the field,…

High Energy Astrophysical Phenomena · Physics 2014-04-09 I. Myserlis , E. Angelakis , L. Fuhrmann , V. Pavlidou , I. Nestoras , V. Karamanavis , A. Kraus , J. A. Zensus

The recent detection of gamma-ray emission from four radio-loud narrow-line Seyfert 1 galaxies suggests that the engine driving the AGN activity of these objects share some similarities with that of blazars, namely the presence of a…

High Energy Astrophysical Phenomena · Physics 2015-05-20 G. Calderone , L. Foschini , G. Ghisellini , M. Colpi , L. Maraschi , F. Tavecchio , R. Decarli , G. Tagliaferri