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Related papers: Issues in Blazar Research

200 papers

The close relation between ground-based TeV observations and satellite borne $\gamma$-ray measurements has been important for the understanding of blazars. The observations which involve the TeV component in blazar studies are reviewed.

This review covers some of the developments in basic theory of astronomical masers over the past ten years. Topics included are the effects of three dimensional geometry and polarization, with special emphasis on the differences between…

Astrophysics · Physics 2007-05-23 Moshe Elitzur

We present the results of our methods to "mine" the blazar sky, i.e., select blazar candidates with very high efficiency. These are based on the cross-correlation between public radio and X-ray catalogs and have resulted in two surveys, the…

Astrophysics · Physics 2009-10-31 Paolo Padovani , Paolo Giommi

Blazars are active galactic nuclei with relativistic jets pointed almost directly at Earth. Blazars are characterized by strong, apparently stochastic flux variability at virtually all observed wavelengths and timescales, from minutes to…

High Energy Astrophysical Phenomena · Physics 2023-02-16 Aryeh Brill

We present multifrequency Very Long Baseline Array (VLBA) observations of J16021+3326. These observations, along with variability data obtained from the Owens Valley Radio Observatory (OVRO) candidate gamma-ray blazar monitoring program,…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 S. E. Tremblay , G. B. Taylor , J. L. Richards , A. C. S. Readhead , J. F. Helmboldt , R. W. Romani , S. E. Healey

The observed spectra of blazars, their intrinsic emission, and the underlying populations of radiating particles are intimately related. The use of these sources as probes of the extragalactic infrared background, a prospect propelled by…

Astrophysics · Physics 2009-11-13 Floyd W. Stecker , Matthew G. Baring , Errol J. Summerlin

I discuss the spectral energy distribution (SED) of all blazars with redshift detected by the {\it Fermi} satellite and listed in the 3LAC catalog. I will update the so called "blazar sequence" from the phenomenological point of view, with…

High Energy Astrophysical Phenomena · Physics 2016-09-28 Gabriele Ghisellini

Jets, paving their way outward through the inner regions of active nuclei, Compton-interact with the UV radiation from an accretion disc and broad emission line region. We calculate the predicted properties of the resulting spectral…

Astrophysics · Physics 2007-05-23 Marek Sikora , Greg Madejski

This report on Photon Colliders briefly reviews three main issues: physics motivation, possible parameters and technical feasibility, plans of works and international cooperation. New scheme of laser optics at the interaction region is…

High Energy Physics - Experiment · Physics 2011-01-13 Valery Telnov

This article reviews and discusses 1) the discovery and early work on the evolution of quasars and AGNs, 2) the different techniques used to find quasars and their suitability for evolutionary studies, 3) the current status of our knowledge…

Astrophysics · Physics 2007-05-23 Patrick S. Osmer

An increasing number of blazars have been reported to show jet wobbling (i.e., non-regular rotations of the structural position angle of their innermost jets in the plane of the sky with amplitudes between 20 deg. and 50 deg., and time…

Astrophysics · Physics 2008-03-25 I. Agudo

The INTEGRAL mission has played a major role in blazar science, thanks to its sensitive coverage of a spectral region (3-100 keV) that is critical for this type of sources, to its flexibility of scheduling and to the large field of view of…

High Energy Astrophysical Phenomena · Physics 2017-03-28 Elena Pian

The broad band sensitivity and flexibility of the BeppoSAX satellite have allowed unprecedented studies of the X-ray emission from blazars. Here we focus on recent results on the SEDs of a group of blazars with emission lines, allowing to…

Astrophysics · Physics 2007-05-23 L. Maraschi , F. Tavecchio

Simultaneous observations of blazars in different spectral regimes imply that the amplitude of variability depends on the observational band. Both in the low energy spectral component and in the high energy spectral component, the amplitude…

Astrophysics · Physics 2007-05-23 Marek Sikora , Greg Madejski , Mitchell Begelman

The knowledge of the structure of the magnetic field inside a blazar jet, as deduced from polarization observations at radio to optical wavelengths, is closely related to the formation and propagation of relativistic jets that result from…

High Energy Astrophysical Phenomena · Physics 2016-10-24 Manasvita Joshi , Alan P. Marscher , Markus Boettcher

Blazars dominate the extragalactic $\gamma$-ray sky and show pronounced flares. Using public Fermi-LAT light curves for 732 blazars with secure redshifts, I implement an automated pipeline to identify and characterize $\gamma$-ray bursts…

High Energy Astrophysical Phenomena · Physics 2025-08-29 Matteo Cerruti

Blazars exhibit multiwavelength variability, a phenomenon whose underlying mechanisms remain elusive. This study investigates the origin of such variability through leptonic blazar emission simulations, focusing on stochastic fluctuations…

High Energy Astrophysical Phenomena · Physics 2024-09-10 Hannes Thiersen , Michael Zacharias , Markus Böttcher

This study explores the origins of cosmic rays and their secondary messengers, focusing on the potential role of four BL Lacs W Comae, 1ES 1959+650, PKS 2005-489, and PKS 2155-304 as potential sources of astrophysical neutrinos and gamma…

High Energy Astrophysical Phenomena · Physics 2025-01-17 Rodrigo Sasse , Rubens Jr. Costa , Luiz A. Stuani Pereira , Rita C. dos Anjos

We describe a uniform all-sky survey of bright blazars, selected primarily by their flat radio spectra, that is designed to provide a large catalog of likely gamma-ray AGN. The defined sample has 1625 targets with radio and X-ray properties…

The empirical relations in the black hole-accretion disk-relativistic jet system and physical processes behind these relations are still poorly understood, partly because they operate close to the black hole within the central light year.…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Tigran G. Arshakian , Vahram Chavushyan
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