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The Energetic Gamma-Ray Experiment Telescope (EGRET) on the Compton Gamma-Ray Observatory (CGRO) discovered gamma-ray emission from more than 67 blazars during its 9 yr lifetime. We conducted an exhaustive search of the EGRET archives and…

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

We fit the spectral energy distributions (SEDs) of members of a large sample of Fermi 2LAC blazars to synchrotron and inverse Compton (IC) models. Our main results are as follows. (i) As suggested by previous works, the correlation between…

High Energy Astrophysical Phenomena · Physics 2016-10-12 R. Xue , D. Luo , L. M. Du , Z. R. Wang , Z. H. Xie , T. F. Yi , D. R. Xiong , Y. B. Xu , W. G. Liu , X. L. Yu

The extragalactic $\gamma$-ray sky is dominated by blazars and their study plays an important role in understanding jet physics, cosmic evolution history and origin of ultra high energy cosmic rays. In this work, we study a large sample of…

High Energy Astrophysical Phenomena · Physics 2022-05-23 Muhammad Shahzad Anjum , Liang Chen , Minfeng Gu

We study a sample of 30 high-redshift blazars ($z>2.5$) by means of spectra and the radiation mechanism with Fermi Large Area Telescope $\gamma$-ray observations spanning 15 years. Three models -- the power law, power law with an…

High Energy Astrophysical Phenomena · Physics 2025-01-27 Fan Wu , Benzhong Dai

Blazar emission models based on magnetic reconnection succeed in reproducing many observed spectral and temporal features, including the short-duration luminous flaring events. Plasmoids, a self-consistent by-product of the tearing…

High Energy Astrophysical Phenomena · Physics 2020-01-08 I. M. Christie , M. Petropoulou , L. Sironi , D. Giannios

We study the correlation between gamma-ray and radio band radiation for 123 blazars, using the Fermi-LAT first source catalog (1FGL) and the RATAN-600 data obtained at the same period of time (within a few months). We found an apparent…

High Energy Astrophysical Phenomena · Physics 2015-05-20 T. Mufakharov , M. Mingaliev , Yu. Sotnikova , Ya. Naiden , A. Erkenov

In this paper we develop the extended jet model of Potter & Cotter to model the simultaneous multi-wavelength spectra of six Compton-dominant blazars. We include an accelerating parabolic base transitioning to a slowly decelerating conical…

High Energy Astrophysical Phenomena · Physics 2015-06-15 William J. Potter , Garret Cotter

Beaming effect is important for the observational properties of blazars. In this work, we collect 91 $Fermi$ blazars with available radio Doppler factors. $\gamma$-ray Doppler factors are estimated and compared with radio Doppler factors…

High Energy Astrophysical Phenomena · Physics 2017-07-19 C. Lin , J. H. Fan , H. B. Xiao

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 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

Single-zone synchrotron self-Compton and external Compton models are widely used to explain broad-band Spectral Energy Distributions (SEDs) of blazars from infrared to gamma-rays. These models bear obvious similarities to the homogeneous…

The blazar AO 0235+164 (z = 0.94) has been one of the most active objects observed by Fermi Large Area Telescope (LAT) since its launch in Summer 2008. In addition to the continuous coverage by Fermi, contemporaneous observations were…

High Energy Astrophysical Phenomena · Physics 2012-07-13 M. Ackermann , M. Ajello , J. Ballet , G. Barbiellini , D. Bastieri , R. Bellazzini , R. D. Blandford , E. D. Bloom , E. Bonamente , A. W. Borgland , E. Bottacini , J. Bregeon , M. Brigida , P. Bruel , R. Buehler , S. Buson , G. A. Caliandro , R. A. Cameron , P. A. Caraveo , J. M. Casandjian , E. Cavazzuti , C. Cecchi , E. Charles , A. Chekhtman , J. Chiang , S. Ciprini , R. Claus , J. Cohen-Tanugi , S. Cutini , F. D'Ammando , F. de Palma , C. D. Dermer , E. do Couto e Silva , P. S. Drell , A. Drlica-Wagner , R. Dubois , C. Favuzzi , S. J. Fegan , E. C. Ferrara , W. B. Focke , P. Fortin , L. Fuhrmann , Y. Fukazawa , P. Fusco , F. Gargano , D. Gasparrini , N. Gehrels , S. Germani , N. Giglietto , P. Giommi , F. Giordano , M. Giroletti , T. Glanzman , G. Godfrey , I. A. Grenier , S. Guiriec , D. Hadasch , M. Hayashida , R. E. Hughes , R. Itoh , G. Johannesson , A. S. Johnson , H. Katagiri , J. Kataoka , J. Knodlseder , M. Kuss , J. Lande , S. Larsson , S. -H. Lee , F. Longo , F. Loparco , B. Lott , M. N. Lovellette , P. Lubrano , G. M. Madejski , M. N. Mazziotta , J. E. McEnery , J. Mehault , P. F. Michelson , W. Mitthumsiri , T. Mizuno , C. Monte , M. E. Monzani , A. Morselli , I. V. Moskalenko , S. Murgia , M. Naumann-Godo , S. Nishino , J. P. Norris , E. Nuss , T. Ohsugi , A. Okumura , N. Omodei , E. Orlando , M. Ozaki , D. Paneque , J. H. Panetta , V. Pelassa , M. Pesce-Rollins , M. Pierbattista , F. Piron , G. Pivato , T. A. Porter , S. Raino , R. Rando , D. Rastawicki , M. Razzano , A. Readhead , A. Reimer , O. Reimer , L. C. Reyes , J. L. Richards , C. Sbarra , C. Sgro , E. J. Siskind , G. Spandre , P. Spinelli , A. Szostek , H. Takahashi , T. Tanaka , J. G. Thayer , J. B. Thayer , D. J. Thompson , M. Tinivella , D. F. Torres , G. Tosti , E. Troja , T. L. Usher , J. Vandenbroucke , V. Vasileiou , G. Vianello , V. Vitale , A. P. Waite , B. L. Winer , K. S. Wood , Z. Yang , S. Zimmer , R. Moderski , K. Nalewajko , M. Sikora , M. Villata , C. M. Raiteri , H. D. Aller , M. F. Aller , A. A. Arkharov , E. Benitez , A. Berdyugin , D. A. Blinov , M. Boettcher , O. J. A. Bravo Calle , C. S. Buemi , D. Carosati , W. P. Chen , C. Diltz , A. Di Paola , M. Dolci , N. V. Efimova , E. Forn\' , M. A. Gurwell , J. Heidt , D. Hiriart , B. Jordan , G. Kimeridze , T. S. Konstantinova , E. N. Kopatskaya , E. Koptelova , O. M. Kurtanidze , A. Lahteenmaki , E. G. Larionova , L. V. Larionova , V. M. Larionov , P. Leto , E. Lindfors , H. C. Lin , D. A. Morozova , M. G. Nikolashvili , K. Nilsson , M. Oksman , P. Roustazadeh , A. Sievers , L. A. Sigua , A. Sillanpaa , T. Takahashi , L. O. Takalo , M. Tornikoski , C. Trigilio , I. S. Troitsky , G. Umana , E. Angelakis , T. P. Krichbaum , I. Nestoras , D. Riquelme , M. Krips , S. Trippe , A. Arai , K. S. Kawabata , K. Sakimoto , M. Sasada , S. Sato , M. Uemura , M. Yamanaka , M. Yoshida , T. Belloni , G. Tagliaferri , E. W. Bonning , J. Isler , C. M. Urry , E. Hoversten , A. Falcone , C. Pagani , M. Stroh

The non-thermal spectra of jetted active galactic nuclei show a variety of shapes in their low- and high energy components. In some of the brightest Fermi-LAT blazars, prominent spectral breaks at a few GeV have been regularly detected,…

High Energy Astrophysical Phenomena · Physics 2016-04-20 Lars Hunger , Anita Reimer

The physics-determined broadband spectral energy distributions (SEDs) of blazars have been widely used to study the property during their flaring/outburst states, while the non-flaring state takes up most of their lifetime and the general…

High Energy Astrophysical Phenomena · Physics 2025-09-16 Hubing Xiao , Haitao Cao , Rui Xue , Zhihao Ouyang , Shaohua Zhang , Junping Chen , Zhijian Luo , Jianghe Yang , Junhui Fan

The second-order Fermi acceleration (Fermi-II) driven by turbulence may be responsible for the electron acceleration in blazar jets. We test this model with time-dependent simulations. The hard electron spectrum predicted by the Fermi-II…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Katsuaki Asano , Fumio Takahara , Masaaki Kusunose , Kenji Toma , Jun Kakuwa

Observations of blazar flaring states reveal remarkably different variability time scales. Especially rapid flares with flux doubling time scales of the order of minutes have been puzzling for quite some time. Many modeling attempts use the…

High Energy Astrophysical Phenomena · Physics 2015-06-11 Michael Zacharias , Reinhard Schlickeiser

We utilized a sample from the Fermi-LAT 14-year Source Catalog by adjusting the flux detection threshold, enabling us to derive the intrinsic source count distribution $dN/dF_{25}$ of extragalactic blazars using nonparametric, unbinned…

High Energy Astrophysical Phenomena · Physics 2024-08-28 Xuhang Yin , Houdun Zeng

We study the relation between the mass accretion rate, the jet power, and the black hole mass of blazars. To this aim, we make use of the Sloan Digital Sky Survey (SDSS) and the 11 months catalog of blazars detected at energies larger than…

High Energy Astrophysical Phenomena · Physics 2012-05-18 T. Sbarrato , G. Ghisellini , L. Maraschi , M. Colpi

The Fermi satellite has been reporting the detailed temporal properties of gamma-ray bursts (GRBs) in an extremely broad spectral range, 8 keV - 300 GeV, in particular, the unexpected delays of the GeV emission onsets behind the MeV…

High Energy Astrophysical Phenomena · Physics 2009-12-18 Kenji Toma , Xue-Feng Wu , Peter Meszaros