English
Related papers

Related papers: Monitoring the Extragalactic High Energy Sky

200 papers

Context: Being dominated by non-thermal emission from aligned relativistic jets, blazars allow us to elucidate the physics of extragalactic jets, and, ltimately, how the energy is extracted from the central black hole in radio-loud active…

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

High-energy solar flares have shown to have at least two distinct phases: prompt-impulsive and delayed-gradual. Identifying the mechanism responsible for accelerating the electrons and ions and the site at which it occurs during these two…

Solar and Stellar Astrophysics · Physics 2021-09-29 Melissa Pesce-Rollins , Nicola Omodei , Vahe' Petrosian , Francesco Longo

The Universe is largely transparent to $\gamma$ rays in the GeV energy range, making these high-energy photons valuable for exploring energetic processes in the cosmos. After seven years of operation, the Fermi {\it Gamma-ray Space…

High Energy Astrophysical Phenomena · Physics 2016-01-20 F. Massaro , D. J. Thompson , E. C. Ferrara

The launching mechanism of the jets of active galactic nuclei is observationally poorly constrained, due to the large distances to these objects and the very small scales (sub-parsec) involved. In order to better constrain theoretical…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 I. Marti-Vidal , S. Muller , F. Combes , S. Aalto , A. Beelen , J. Darling , M. Guelin , C. Henkel , C. Horellou , J. M. Marcaide , S. Martin , K. M. Menten , Dinh-V-Trung , M. Zwaan

High-redshift blazars are among the most powerful objects in the Universe. The spectral and temporal properties of thirty-three distant blazars ($z>2.5$) detected in the high energy $\gamma$-ray band are investigated by analyzing the {\it…

High Energy Astrophysical Phenomena · Physics 2020-08-25 N. Sahakyan , D. Israyelyan , G. Harutyunyan , M. Khachatryan , S. Gasparyan

We compute the contribution of blazars (Flat Spectrum Radio Quasars and BL-Lacs) to the Fermi-LAT Extragalactic gamma-ray Background, assuming a gamma-ray luminosity function proportional to the luminosity function of radio galaxies and the…

High Energy Astrophysical Phenomena · Physics 2011-11-01 Massimo Cavadini , Ruben Salvaterra , Francesco Haardt

The Extragalactic Background Light (EBL) from the infrared (IR) through the ultraviolet (UV) is dominated by emission from stars, either directly or through absorption and reradiation by dust. It can thus give information on the star…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-14 Justin D. Finke

VERITAS is an array of four 12-m atmospheric Cherenkov telescopes, designed to observe the very-high-energy (VHE; E $\geq$100 GeV) sky. Since 2007, it has detected more than 20 extra-galactic sources, the majority of which are…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Matteo Cerruti

High redshift blazars are among the most powerful non-explosive sources in the Universe and play a crucial role in understanding the evolution of relativistic jets. To understand these bright objects, we performed a detailed investigation…

High Energy Astrophysical Phenomena · Physics 2024-01-29 N. Sahakyan , G. Harutyunyan , S. Gasparyan , D. Israyelyan

High-redshift ($z >3$) $\gamma$-ray blazars are rare, but they are crucial for our understanding of jet evolution, $\gamma$-ray production and propagation, and the growth of supermassive black holes in the early universe. A new analysis of…

High Energy Astrophysical Phenomena · Physics 2024-06-07 Hai Lei , Ying-Kang Zhang , Xiong Jiang , Sebastian Kiehlmann , Anthony C. S. Readhead , Liang Chen , Neng-Hui Liao , Tao An

With their jet pointing towards us, blazars are ideal tools to study the physics and structure of extragalactic jets. Their powerful jets are cosmic particle accelerators and are alleged to be one of the production sites of the high-energy…

High Energy Astrophysical Phenomena · Physics 2025-11-25 Claudia M. Raiteri

The radio properties of blazars detected by the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope have been observed contemporaneously by the Very Long Baseline Array (VLBA). In total, 232 sources were observed with…

Blazars, one of the most extreme class of active galaxies, constitute so far the largest known population of $\gamma$-ray sources and their number is continuously growing in the Fermi catalogs. However in the latest release of the Fermi…

The global contribution of unresolved gamma-ray point sources to the extragalactic gamma-ray background has been recently measured down to gamma-ray fluxes lower than those reached with standard source detection techniques, and by employing…

High Energy Astrophysical Phenomena · Physics 2020-05-27 Silvia Manconi , Michael Korsmeier , Fiorenza Donato , Nicolao Fornengo , Marco Regis , Hannes Zechlin

We report the detection of a new gamma-ray source in the Fermi-LAT sky using a source detection tool based on the Minimal Spanning Tree algorithm. The source, not reported in previous LAT catalogues but very recently observed in the X-rays…

High Energy Astrophysical Phenomena · Physics 2015-06-12 E. Bernieri , R. Campana , E. Massaro , A. Paggi , A. Tramacere

The intermediate-frequency-peaked BL Lac object 3C 66A was detected in a flaring state by the Fermi-LAT and VERITAS observatories in October 2008. These data and follow-up observations at other wavelengths create a rich sample of light…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Luis C. Reyes

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

Using blazar light curves from the optical All-Sky Automated Survey for Supernovae (ASAS-SN) and the $\gamma$-ray \textit{Fermi}-LAT telescope, we performed the most extensive statistical correlation study between both bands, using a sample…

High Energy Astrophysical Phenomena · Physics 2023-01-18 T. de Jaeger , B. J. Shappee , C. S. Kochanek , J. T. Hinkle , S. Garrappa , I. Liodakis , A. Franckowiak , K. Z. Stanek , J. F. Beacom , J. L. Prieto

The Fermi-LAT has observed new gamma-ray flares from the blazar B0218+357 during July 2014. While no significant change in the gamma-ray spectrum has been previously observed through the flaring phase in late-2012, during this recent high…

High Energy Astrophysical Phenomena · Physics 2015-02-12 S. Buson , C. C. Cheung , S. Larsson , J. D. Scargle
‹ Prev 1 4 5 6 7 8 10 Next ›