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Aims. The observation of gamma -ray flares from blazar 0836+710 in 2011, following a period of quiescence, offered an opportunity to study correlated activity at different wavelengths for a high-redshift (z=2.218) active galactic nucleus.…

High Energy Astrophysical Phenomena · Physics 2015-06-16 A. Akyuz , D. J. Thompson , D. Donato , J. S. Perkins , L. Fuhrmann , E. Angelakis , J. A. Zensus , S. Larsson , K. Sokolovsky , O. Kurtanidze

The internal-shocks scenario in relativistic jets has been used to explain the variability of blazars' outflow emission. Recent simulations have shown that the magnetic field alters the dynamics of these shocks producing a whole zoo of…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Jesus M. Rueda-Becerril , Petar Mimica , Miguel A. Aloy , Carmen Aloy

The evidence for joint gamma and neutrino emission from the blazar TXS 0506+056 has renewed interest in blazars as neutrino sources. The detection of neutrinos from blazars can be seen as the smoking gun for the presence of relativistic…

High Energy Astrophysical Phenomena · Physics 2020-05-20 Matteo Cerruti

We investigate the previously proposed possibility that multi-epoch broadband polarimetry could act as a complement or limited proxy for VLBI observations of blazars, in that the number of polarised emission components in the jet, and some…

Astrophysics of Galaxies · Physics 2019-02-20 C. S. Anderson , S. P. O'Sullivan , G. H. Heald , T. Hodgson , A. Pasetto , B. M. Gaensler

The multi-wavelength spectral and temporal variability observed in blazars set tight constraints on current theoretical emission models. Here, we investigate the relativistic magnetic reconnection process as a source of blazar emission in…

High Energy Astrophysical Phenomena · Physics 2018-12-04 I. M. Christie , M. Petropoulou , L. Sironi , D. Giannios

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

Typical blazars seem to be associated with FR I and FR II radio galaxies and radio-loud quasars. However, what happens at lower powers? Do blazars exist in low-luminosity AGN or do they exist in radio-quiet AGN? A recent detection of…

Astrophysics · Physics 2007-05-23 Heino Falcke , Sera Markoff , Peter L. Biermann

Densely time sampled multi-frequency flux measurements of the extreme BL Lac object S5 0716+714 over the past three years allow us to study its broad-band variability, and the detailed underlying physics, with emphasis on the location and…

High Energy Astrophysical Phenomena · Physics 2019-08-16 B. Rani , T. P. Krichbaum , L. Fuhrmann , B. Lott , M. Boettcher , J. A. Zensus

We propose a scenario where blazars are classified as flat-spectrum radio quasars (FSRQs), BL Lacs, low synchrotron, or high synchrotron peaked objects according to a varying mix of the Doppler boosted radiation from the jet, the emission…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 P. Giommi , P. Padovani , G. Polenta , S. Turriziani , V. D'Elia , S. Piranomonte

We investigate the dependence of gamma-ray brightness of blazars on intrinsic properties of their parsec-scale radio jets and the implication for relativistic beaming. By combining apparent jet speeds derived from high-resolution VLBA…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 T. Savolainen , D. C. Homan , T. Hovatta , M. Kadler , Y. Y. Kovalev , M. L. Lister , E. Ros , J. A. Zensus

We present a model in which AGN jets are described by a dense series of plasma blobs, distributed in masses and velocities. The blobs expand and collide, and ultimately form a continuous jet flow as observed on larger scales. When blobs…

High Energy Astrophysical Phenomena · Physics 2010-07-27 Jörg P. Rachen , Max Häberlein , Felix Reimold , Thomas Krichbaum

PKS 2155--304 is one of the brightest blazars in the X-ray band. It was repeatedly monitored with BeppoSax during three long campaigns of about 2 days each in November of 1996, 1997 and 1999. The source underwent different states of…

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

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

We study the expected variability patterns of blazars within the two-zone acceleration model putting special emphasis on flare shapes and spectral lags. We solve semi-analytically the kinetic equations which describe the particle evolution…

High Energy Astrophysical Phenomena · Physics 2015-05-20 K. Moraitis , A. Mastichiadis

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…

We describe new implementations of leptonic and hadronic models for the broadband emission from relativistic jets in AGN in a temporary steady state. For the leptonic model, a temporary equilibrium between particle injection/acceleration,…

High Energy Astrophysical Phenomena · Physics 2015-06-15 M. Boettcher , A. Reimer , K. Sweeney , A. Prakash

Violent multi-wavelength variabilities are observed in gamma-ray-selected blazars. We present an analysis of long-term light curves for eight bright blazars to explore the co-variation pattern in the gamma-ray and radio bands. We extract…

High Energy Astrophysical Phenomena · Physics 2020-05-27 Hai-Ming Zhang , Zhen-Jie Wang , Jin Zhang , Ting-Feng Yi , Liang Chen , Rui-Jing Lu , En-Wei Liang

Since mid-2007 we have carried out a dedicated long-term monitoring programme at 15 GHz using the Owens Valley Radio Observatory 40 meter telescope. One of the main goals of this programme is to study the relation between the radio and…

High Energy Astrophysical Phenomena · Physics 2015-06-23 W. Max-Moerbeck , J. L. Richards , T. Hovatta , V. Pavlidou , T. J. Pearson , A. C. S. Readhead , O. G. King , R. Reeves

We report on the findings of a 364 ksec observation of the BL LAC object Mrk 421 with the X-ray observatory Suzaku. The analysis in this paper uses fluxes and hardness ratios in the broad energy range from 0.5 keV to 30 keV. During the…

High Energy Astrophysical Phenomena · Physics 2015-05-19 Alfred B. Garson , Matthew G. Baring , Henric Krawczynski