English
Related papers

Related papers: Variability along the Blazar-Sequence - Hints for …

200 papers

The BL Lac object Mkn 501, one of the only three extragalactic sources (with Mkn 421 and 1ES 2344+514) so far detected at TeV energies, was observed with the BeppoSAX satellite on 7, 11, and 16 April 1997 during a phase of high activity at…

While blazars have long been one of the candidates in the search for the origin of ultra-high energy cosmic rays and astrophysical neutrinos, the BL Lac object TXS 0506+056 is the first extragalactic source that is correlated with some…

High Energy Astrophysical Phenomena · Physics 2018-10-23 M. Cerruti , A. Zech , C. Boisson , G. Emery , S. Inoue , J. -P. Lenain

Blazars, a subclass of active galactic nuclei (AGN), are known to be bright $\gamma$-ray sources, frequently exhibiting active (flaring) periods. The blazar PKS~2155-304 is a high synchrotron-peaked BL Lac object located at redshift…

High Energy Astrophysical Phenomena · Physics 2024-02-26 Hong-Bin Tan , Ruo-Yu Liu , Markus Böttcher

We present a first systematic time series study of a sample of blazars observed by the Transiting Exoplanet Survey Satellite $\textit{TESS}$ spacecraft. By cross matching the positions of the sources in the TESS observations with those from…

High Energy Astrophysical Phenomena · Physics 2022-11-23 Vivek Reddy Pininti , Gopal Bhatta , Sagarika Paul , Aman Kumar , Aayushi Rajgor , Rahul Barnwal , Sarvesh Gharat

{We focus on characterizing the high-energy emission mechanisms of blazars by analyzing the variability in the radio band of the light curves of more than a thousand sources. We are interested in assigning complexity parameters to these…

Data Analysis, Statistics and Probability · Physics 2022-05-11 Belén Acosta-Tripailao , Walter Max-Moerbeck , Denisse Pastén , Pablo S. Moya

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

Extreme high-energy peaked BL Lac objects (EHBLs) are blazars whose synchrotron emission peaks at exceptionally high energies, above few keV, in the hard X-ray regime. So far, only a handful of those objects has been detected at very high…

Blazars emit across all electromagnetic wavelengths. While the so-called one-zone model has described well both quiescent and flaring states, it cannot explain the radio emission and fails in more complex data sets, such as AP Librae. In…

High Energy Astrophysical Phenomena · Physics 2023-07-10 Michael Zacharias , Anita Reimer , Catherine Boisson , Andreas Zech

Blazars - active galaxies with the jet pointing at Earth - emit across all electromagnetic wavelengths. The so-called one-zone model has described well both quiescent and flaring states, however it cannot explain the radio emission. In…

High Energy Astrophysical Phenomena · Physics 2021-08-03 Michael Zacharias , Anita Reimer , Andreas Zech

Blazars are active galactic nuclei with their relativistic jets pointing toward the observer, with two major sub-classes, the flat spectrum radio quasars and BL Lac objects. We present multi-wavelength photometric and spectroscopic…

Blazar spectra are one of the most important windows into the physical processes occurring along jets. The spectrum, composed from the different emitting regions along the jet, allows us to constrain the physical conditions in the jet. I…

High Energy Astrophysical Phenomena · Physics 2015-06-17 William J. Potter , Garret Cotter

Flux distribution is an important tool to understand the variability processes in active galactic nuclei. We now have available a great deal of observational evidences pointing towards the presence of log-normal components in the high…

High Energy Astrophysical Phenomena · Physics 2018-12-18 Carlo Romoli , Nachiketa Chakraborty , Daniela Dorner , Andrew M. Taylor , Michael Blank

The BL Lac object PKS 0735+178 was in its historic $\gamma$-ray brightness state during December 2021. This period also coincides with the detection of a neutrino event IC211208A, which was localized close to the vicinity of PKS 0735+178.…

High Energy Astrophysical Phenomena · Physics 2024-01-24 Athira M Bharathan , C. S. Stalin , S. Sahayanathan , Subir Bhattacharyya , Blesson Mathew

We present the results of six BeppoSAX observations of 1ES 2344+514, five of which were taken within a week. 1ES 2344+514, one of the few known TeV BL Lac objects, was detected by the BeppoSAX Narrow Field Instruments between 0.1 to \~50…

Astrophysics · Physics 2009-10-31 P. Giommi , P. Padovani , E. Perlman

Three independent predictions follow from postulating the existence of protons co-accelerated with electrons in extragalactic jets (i) multi-TeV gamma ray emission from nearby blazars, (ii) extragalactic cosmic ray protons up to 10^20 eV,…

Astrophysics · Physics 2009-10-31 Karl Mannheim

We use the distributions of spectral indices of a large homogenous sample of Fermi-detected blazars to re-investigate the relationship between flat spectrum radio quasars (FSRQs) and subclasses of BL Lac objects (BL Lacs). We compute the…

High Energy Astrophysical Phenomena · Physics 2020-07-20 E. U. Iyida , F. C. Odo , A. E. Chukwude , A. A. Ubachukwu

The gamma-ray emission offers a powerful diagnostic tool to probe jets and their surroundings in flat spectrum radio quasars (FSRQ). In particular, sources emitting at high energies (>10 GeV) give us the strongest constraints. This…

High Energy Astrophysical Phenomena · Physics 2015-06-18 L. Pacciani , F. Tavecchio , I. Donnarumma , A. Stamerra , L. Carrasco , E. Recillas , A. Porras , M. Uemura

Spectral fitting of the radio through hard X-ray emission of BL Lac objects has previously been used to predict their level of high-energy (GeV - TeV) emission. In this paper, we point out that such spectral fitting can have very large…

Astrophysics · Physics 2009-11-07 M. Boettcher , R. Mukherjee , A. Reimer

We report on multiwavelength target-of-opportunity observations of the blazar PKS 0735+178, located 2.2$^\circ$ away from the best-fit position of the IceCube neutrino event IceCube-211208A detected on December 8, 2021. The source was in a…

High Energy Astrophysical Phenomena · Physics 2023-07-03 A. Acharyya , C. B. Adams , A. Archer , P. Bangale , J. T. Bartkoske , P. Batista , W. Benbow , A. Brill , J. H. Buckley , J. L. Christiansen , A. J. Chromey , M. Errando , A. Falcone , Q. Feng , G. M. Foote , L. Fortson , A. Furniss , G. Gallagher , W. Hanlon , D. Hanna , O. Hervet , C. E. Hinrichs , J. Hoang , J. Holder , T. B. Humensky , W. Jin , P. Kaaret , M. Kertzman , M. Kherlakian , D. Kieda , T. K. Kleiner , N. Korzoun , S. Kumar , M. J. Lang , M. Lundy , G. Maier , C. E McGrath , M. J. Millard , J. Millis , C. L. Mooney , P. Moriarty , R. Mukherjee , S. O'Brien , R. A. Ong , M. Pohl , E. Pueschel , J. Quinn , K. Ragan , P. T. Reynolds , D. Ribeiro , E. Roache , I. Sadeh , A. C. Sadun , L. Saha , M. Santander , G. H. Sembroski , R. Shang , M. Splettstoesser , A. Kaushik Talluri , J. V. Tucci , V. V. Vassiliev , A. Weinstein , D. A. Williams , S. L. Wong , J. Woo , F. Aharonian , J. Aschersleben , M. Backes , V. Barbosa Martins , R. Batzofin , Y. Becherini , D. Berge , K. Bernlohr , B. Bi , M. Bottcher , C. Boisson , J. Bolmont , M. de Bony de Lavergne , J. Borowska , M. Bouyahiaoui , F. Bradascio , M. Breuhaus , R. Brose , F. Brun , B. Bruno , T. Bulik , C. Burger-Scheidlin , S. Caroff , S. Casanova , R. Cecil , J. Celic , M. Cerruti , T. Chand , S. Chandra , A. Chen , J. Chibueze , O. Chibueze , G. Cotter , S. Dai , J. Damascene Mbarubucyeye , A. Djannati-Atai , A. Dmytriiev , V. Doroshenko , S. Einecke , J. -P. Ernenwein , G. Fichet de Clairfontaine , M. Filipovic , G. Fontaine , M. Fussling , S. Funk , S. Gabici , S. Ghafourizadeh , G. Giavitto , D. Glawion , J. F. Glicenstein , P. Goswami , G. Grolleron , L. Haerer , J. A. Hinton , T. L. Holch , M. Holler , D. Horns , M. Jamrozy , F. Jankowsky , V. Joshi , I. Jung-Richardt , E. Kasai , K. Katarzynski , R. Khatoon , B. Khelifi , S. Klepser , W. Kluzniak , K. Kosack , D. Kostunin , R. G. Lang , S. Le Stum , A. Lemiere , J. P. Lenain , F. Leuschner , T. Lohse , A. Luashvili , I. Lypova , J. Mackey , D. Malyshev , V. Marandon , P. Marchegiani , A. Marcowith , G. Marti-Devesa , R. Marx , A. Mitchell , R. Moderski , L. Mohrmann , A. Montanari , E. Moulin , T. Murach , K. Nakashima , J. Niemiec , A. Priyana Noel , P. O'Brien , L. Olivera-Nieto , E. de Ona Wilhelmi , M. Ostrowski , S. Panny , M. Panter , G. Peron , D. A. Prokhorov , G. Puhlhofer , M. Punch , A. Quirrenbach , P. Reichherzer , A. Reimer , O. Reimer , H. Ren , M. Renaud , F. Rieger , B. Rudak , E. Ruiz-Velasco , V. Sahakian , A. Santangelo , M. Sasaki , J. Schafer , F. Schussler , H. M. Schutte , U. Schwanke , J. N. S. Shapopi , A. Specovius , S. Spencer , L. Stawarz , R. Steenkamp , S. Steinmassl , I. Sushch , H. Suzuki , T. Takahashi , T. Tanaka , R. Terrier , C. van Eldik , M. Vecchi , J. Veh , C. Venter , J. Vink , R. White , A. Wierzcholska , Yu Wun Wong , M. Zacharias , D. Zargaryan , A. A. Zdziarski , A. Zech , S. Zouari , N. Zywucka , K. Mori
‹ Prev 1 8 9 10 Next ›