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Related papers: An Overview of Blazar Variability

200 papers

Blazars display strong variability on multiple timescales and in multiple radiation bands. Their variability is often characterized by power spectral densities (PSDs) and time lags plotted as functions of the Fourier frequency. We develop a…

Astrophysics of Galaxies · Physics 2015-06-19 Justin D. Finke , Peter A. Becker

Blazars are a highly-variable, radio-loud subclass of active galactic nuclei (AGN). In order to better understand such objects we must be able to easily identify candidate blazars from the growing population of unidentified sources. Working…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Philip S. Cowperthwaite , F. Massaro , R. D'Abrusco , A. Paggi , G. Tosti , Howard A. Smith

The extreme variability of blazars, in both timescale and amplitude, is generally explained as the effect of a relativistic jet closely aligned to the observer's line-of-sight. Due to causality arguments, variability characteristics…

We investigate the spectral properties of the brightest gamma-ray flares of blazars detected by the Fermi Large Area Telescope. We search for the presence of spectral breaks and measure the spectral curvature on typical time scales of a few…

High Energy Astrophysical Phenomena · Physics 2015-06-24 Susanna Kohler , Krzysztof Nalewajko

We study the quasi-simultaneous near-IR, optical, UV, and X-ray photometry of eleven gamma-ray selected blazars for which redshift estimates larger than 1.2 have been recently provided. Four of these objects turn out to be high-power…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 P. Padovani , P. Giommi , A. Rau

The hypothesis that AGN jets might be the sources of the ultra-high energy cosmic rays has originally motivated the venture of TeV gamma ray astronomy. Surprisingly, after the discovery of TeV emission from blazars the attention has shifted…

Astrophysics · Physics 2010-12-13 Jorg P. Rachen

Active galactic nuclei are the most luminous persistent (non-transient, even if often variable) objects in the Universe. They are bright in the entire electromagnetic spectrum. Blazars are a special class where the jets point nearly to our…

Astrophysics of Galaxies · Physics 2019-02-21 A. Gemes , K. É. Gabányi , S. Frey , T. An , Z. Paragi , A. Moór

Relativistic jets in AGN in general, and in blazars in particular, are the most energetic and among the most powerful astrophysical objects known so far. Their relativistic nature provides them with the ability to emit profusely at all…

High Energy Astrophysical Phenomena · Physics 2012-10-09 Ivan Agudo , Alan P. Marscher , Svetlana G. Jorstad , Jose L. Gomez

Since 2002, the number of detected blazars at E_\gamma > 100 GeV has more than doubled. I study all currently known BL Lac-type objects with published energy spectra. Their intrinsic energy spectra are reconstructed by removing…

Astrophysics · Physics 2009-01-08 Robert Wagner

Multi-Messenger observations and theory of astrophysical objects is fast becoming a critical research area in the astrophysics scientific community. In particular, point-like objects like that of BL Lac, flat spectrum radio quasars (FSRQ),…

High Energy Astrophysical Phenomena · Physics 2024-05-24 Ronald Gamble , Jordan Forman , Amethyst Barnes , Gokul Srinivasaragavan , Isiah Holt , Marvin Jones

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

We analyse a group of radio sources, a subset of the 200 mJy sample, all of which have core-jet radio structures measured with VLBI and have flat spectra stretching from the radio to the millimetre/sub-millimetre band. Thus the objects have…

Astrophysics · Physics 2009-11-10 S. Anton , I. W. A. Browne

Extremely high-peaked BL Lac objects (or extreme blazars) are unique extragalactic laboratories where particle acceleration processes are pushed at their physical limits. In these blazars, synchrotron emission peaking above keV energies is…

High Energy Astrophysical Phenomena · Physics 2025-10-08 L. Foffano , C. Arcaro , A. Arbet-Engels , F. D'Ammando , P. Da Vela , J. Jormanainen , D. Linder , S. Menon , E. Prandini , S. Ventura , E. Visentin

Blazars, a highly energetic subclass of jetted active galactic nuclei, show a broad band spectral energy distribution (SED) with two bumps, resulting from non-thermal jet emission. In 1998, an anticorrelation between the SED luminosity and…

High Energy Astrophysical Phenomena · Physics 2025-06-24 I. Viale , E. Prandini , C. Righi , F. Bovolon , N. Sahakyan

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

The non-thermal spectra of blazars, observed from radio to GeV/TeV gamma-rays, reveal two pronounced components, both produced by radiation by energetic particles. One peaks in the IR - to soft X-ray band, radiating via the synchrotron…

Astrophysics · Physics 2009-10-31 Tadayuki Takahashi , Greg Madejski , Hidetoshi Kubo

We collect data from the radio to the gamma-ray range for three complete samples of blazars: the Slew Survey and the 1Jy samples of BL Lacs and the 2Jy sample of Flat Spectrum Radio-Loud Quasars (FSRQs). The fraction of objects detected in…

Astrophysics · Physics 2009-10-30 G. Fossati , L. Maraschi , A. Celotti , A. Comastri , G. Ghisellini

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

Relativistic jets of active galactic nuclei have been known to exist for 100 years. Blazars with their jet pointing close to our line of sight are some of the most variable and extreme objects in the universe, showing emission from radio to…

High Energy Astrophysical Phenomena · Physics 2020-08-18 Talvikki Hovatta , Elina Lindfors

Blazars exhibit flares across the electromagnetic spectrum. Many $\gamma$-ray flares are highly correlated with flares detected at optical wavelengths; however, a small subset appears to occur in isolation, with little or no variability…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Nicholas R. MacDonald , Alan P. Marscher , Svetlana G. Jorstad , Manasvita Joshi