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The bright X-ray selected BL Lacertae object PKS 2155-304 has been the target of two intense multiwavelength campaigns, in November 1991 and in May 1994. Although the spectral energy distributions at both epochs were quite similar, the…

Astrophysics · Physics 2009-10-30 Markos Georganopoulos , Alan P. Marscher

Since the launch of the Fermi satellite, BL Lacertae has been moderately active at gamma-rays and optical frequencies until May 2011, when the source started a series of strong flares. The exceptional optical sampling achieved by the…

High Energy Astrophysical Phenomena · Physics 2019-08-14 C. M. Raiteri , M. Villata , F. D'Ammando , V. M. Larionov , M. A. Gurwell , D. O. Mirzaqulov , P. S. Smith

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 present the results of our power spectral analysis for the BL Lac object PKS 0735+178 utilizing the Fermi-LAT survey at high-energy $\gamma$-rays, several ground-based optical telescopes, and single-dish radio telescopes operating at GHz…

High Energy Astrophysical Phenomena · Physics 2017-03-22 Arti Goyal , Lukasz Stawarz , Michal Ostrowski , Valeri Larionov , Gopal-Krishna , Paul J. Wiita , Santosh Joshi , Marian Soida , Ivan Agudo

OT 081 is a well-known, luminous blazar that is remarkably variable in many energy bands. We present the first broadband study of the source which includes very-high-energy (VHE, $E>$100\,GeV) $\gamma$-ray data taken by the MAGIC and…

High Energy Astrophysical Phenomena · Physics 2025-03-06 MAGIC Collaboration , H. Abe , S. Abe , V. A. Acciari , I. Agudo , T. Aniello , S. Ansoldi , L. A. Antonelli , A. Arbet Engels , C. Arcaro , M. Artero , K. Asano , D. Baack , A. Babić , A. Baquero , U. Barres de Almeida , I. Batković , J. Baxter , E. Bernardini , M. Bernardos , J. Bernete , A. Berti , C. Bigongiari , A. Biland , O. Blanch , G. Bonnoli , Ž. Bošnjak , I. Burelli , G. Busetto , A. Campoy-Ordaz , A. Carosi , R. Carosi , M. Carretero-Castrillo , A. J. Castro-Tirado , Y. Chai , A. Cifuentes , S. Cikota , E. Colombo , J. L. Contreras , J. Cortina , S. Covino , G. D'Amico , V. D'Elia , P. Da Vela , F. Dazzi , A. De Angelis , B. De Lotto , A. Del Popolo , M. Delfino , J. Delgado , C. Delgado Mendez , D. Depaoli , F. Di Pierro , L. Di Venere , D. Dominis Prester , A. Donini , D. Dorner , M. Doro , D. Elsaesser , G. Emery , J. Escudero , L. Fariña , A. Fattorini , L. Foffano , L. Font , S. Fukami , Y. Fukazawa , R. J. García López , S. Gasparyan , M. Gaug , J. G. Giesbrecht Paiva , N. Giglietto , F. Giordano , P. Gliwny , R. Grau , J. G. Green , D. Hadasch , A. Hahn , L. Heckmann , J. Herrera , D. Hrupec , M. Hütten , R. Imazawa , T. Inada , R. Iotov , K. Ishio , I. Jiménez Martínez , J. Jormanainen , D. Kerszberg , G. W. Kluge , Y. Kobayashi , H. Kubo , J. Kushida , M. Láinez Lezáun , A. Lamastra , F. Leone , E. Lindfors , L. Linhoff , S. Lombardi , F. Longo , M. López-Moya , A. López-Oramas , S. Loporchio , A. Lorini , B. Machado de Oliveira Fraga , P. Majumdar , M. Makariev , G. Maneva , N. Mang , M. Manganaro , S. Mangano , K. Mannheim , M. Mariotti , M. Martínez , A. Mas-Aguilar , D. Mazin , S. Menchiari , S. Mender , S. Mićanović , D. Miceli , J. M. Miranda , R. Mirzoyan , E. Molina , H. A. Mondal , D. Morcuende , C. Nanci , V. Neustroev , C. Nigro , K. Nishijima , T. Njoh Ekoume , K. Noda , S. Nozaki , Y. Ohtani , J. Otero-Santos , S. Paiano , M. Palatiello , D. Paneque , R. Paoletti , J. M. Paredes , L. Pavletić , M. Persic , M. Pihet , G. Pirola , F. Podobnik , P. G. Prada Moroni , E. Prandini , G. Principe , C. Priyadarshi , W. Rhode , M. Ribó , J. Rico , C. Righi , N. Sahakyan , T. Saito , K. Satalecka , F. G. Saturni , B. Schleicher , K. Schmidt , F. Schmuckermaier , J. L. Schubert , T. Schweizer , J. Sitarek , A. Spolon , A. Stamerra , J. Strišković , D. Strom , Y. Suda , T. Surić , S. Suutarinen , H. Tajima , M. Takahashi , R. Takeishi , F. Tavecchio , P. Temnikov , T. Terzić , M. Teshima , L. Tosti , S. Truzzi , S. Ubach , J. van Scherpenberg , S. Ventura , V. Verguilov , I. Viale , C. F. Vigorito , V. Vitale , R. Walter , T. Yamamoto , Collaborators , : , F. Ait Benkhali , Y. Becherini , B. Bi , M. Böttcher , J. Bolmont , A. Brown , T. Bulik , S. Casanova , T. Chand , S. Chandra , J. Chibueze , O. Chibueze , K. Egberts , S. Einecke , J. -P. Ernenwein , G. Fontaine , S. Gabici , P. Goswami , M. Holler , M. Jamrozy , V. Joshi , E. Kasai , K. Katarzyński , R. Khatoon , B. Khélifi , W. Kluzniak , K. Kosack , S. Le Stum , A. Lemière , R. Marx , R. Moderski , M. O. Moghadam , M. de Naurois , J. Niemiec , P. O'Brien , M. Ostrowski , G. Peron , S. Pita , G. Pühlhofer , A. Quirrenbach , B. Rudak , V. Sahakian , D. A. Sanchez , A. Santangelo , M. Sasaki , H. M. Schutte , M. Seglar-Arroyo , J. N. S. Shapopi , R. Steenkamp , C. Steppa , H. Suzuki , T. Tanaka , M. Tluczykont , C. Venter , S. J. Wagner , A. Wierzcholska , A. A. Zdziarski , N. Żywucka , Fermi-LAT Collaboration , : , J. Becerra González , S. Ciprini , T. M. Venters , MWL collaborators , : , F. D'Ammando , A. Esteban-Gutiérrez , V. Fallah Ramazani , A. V. Filippenko , T. Hovatta , H. Jermak , S. Jorstad , S. Kiehlmann , A. Lähteenmäki , V. M. Larionov , E. Larionova , A. P. Marscher , D. Morozova , W. Max-Moerbeck , A. C. S. Readhead , R. Reeves , I. A. Steele , M. Tornikoski , F. Verrecchia , H. Xiao , W. Zheng

Context. The gamma-ray emitting source WISE J141046.00+740511.2 has been associated with a Fermi-LAT detection by crossmatching with Swift/XRT data. It has shown all the canonical observational characteristics of a BL Lac source, including…

We report on a long-lasting, elevated gamma-ray flux state from VER J0521+211 observed by VERITAS, MAGIC, and Fermi-LAT in 2013 and 2014. The peak integral flux above 200 GeV measured with the nightly-binned light curve is $(8.8 \pm 0.4)…

High Energy Astrophysical Phenomena · Physics 2022-08-10 The VERITAS Collaboration , The MAGIC Collaboration

We present a multi-wavelength study of four high redshift blazars, S5 0014+81 ($z=3.37$), CGRaBS J0225+1846 ($z=2.69$), BZQ J1430+4205 ($z=4.72$), and 3FGL J1656.2$-$3303 ($z=2.40$), using the quasi-simultaneous data from {\it Swift}, {\it…

High Energy Astrophysical Phenomena · Physics 2016-07-06 Vaidehi S. Paliya , M. L. Parker , A. C. Fabian , C. S. Stalin

Using millimeter-very long baseline interferometry (VLBI) observations of the BL Lac object S5 0716+714 from August 2008 to September 2013, we investigate variations in the core flux density and orientation of the sub-parsec scale jet i.e.…

High Energy Astrophysical Phenomena · Physics 2014-11-11 B. Rani , T. P. Krichbaum , A. P. Marscher , S. G. Jorstad , J. A. Hodgson , L. Fuhrmann , J. A. Zensus

We present the first deep VLA radio images of flat-spectrum radio quasars (FSRQ) with multiwavelength emission properties similar to those of BL Lacs with synchrotron X-rays. Our observations of twenty-five of these sources show that their…

Astrophysics · Physics 2009-11-13 Hermine Landt , Eric S. Perlman , Paolo Padovani

The blazar 4C 31.03 recently underwent a major gamma-ray outburst at the beginning of 2023 after a prolonged quiescent phase. Fermi-LAT reported a daily average flux of 5x10^-6 phs cm^-2 s^-1, which is about 60 times its average value. We…

High Energy Astrophysical Phenomena · Physics 2024-04-16 Aminabi Thekkoth , Baheeja C , S Sahayanathan , C D Ravikumar

We report on the gamma-ray activity of the blazar Mrk 501 during the first 480 days of Fermi operation. We find that the average LAT gamma-ray spectrum of Mrk 501 can be well described by a single power-law function with a photon index of…

A majority of blazars exhibit variable emission across the entire electromagnetic spectrum, observed over various time scales. In particular, discernible periodic patterns are detected in the $\gamma$-ray light curves of a few blazars, such…

High Energy Astrophysical Phenomena · Physics 2025-06-18 Alba Rico , A. Domínguez , P. Peñil , M. Ajello , S. Buson , S. Adhikari , M. Movahedifar

In order to study short timescale optical variability of $\gamma$-ray blazar S5 0716+714, quasi-simultaneous spectroscopic and multi-band photometric observations were performed from 2018 November to 2019 March with the 2.4 m optical…

Astrophysics of Galaxies · Physics 2021-01-01 Hai-Cheng. Feng , H. T. Liu , J. M. Bai , L. F. Xing , Y. B. Li , M. Xiao , Y. X. Xin

The $\gamma-$ray emission from flat-spectrum radio quasars (FSRQs) is thought to be dominated by the inverse Compton scattering of the external sources of photon fields, e.g., accretion disk, broad-line region (BLR), and torus. FSRQs show…

High Energy Astrophysical Phenomena · Physics 2022-11-16 Savithri H. Ezhikode , Amit Shukla , Gulab C. Dewangan , Pramod K. Pawar , Sushmita Agarwal , Blesson Mathew , Akhil Krishna R

In this work, a time-dependent modeling is developed to study the emission properties of blazars in the low state. Motivated by various observations, we speculate and assume that numerous discrete radiation zones throughout the jet of a…

High Energy Astrophysical Phenomena · Physics 2023-09-22 Ruo-Yu Liu , Rui Xue , Ze-Rui Wang , Hong-Bin Tan , Markus Böttcher

About twenty years of radio observations in five bands (from 4.8 to 37 GHz) of the BL Lac object GC 0109+224 (S2 0109+22, RGB J0112+227), are presented and analysed together with the optical data. Over the past ten years this blazar has…

Astrophysics · Physics 2016-08-16 Stefano Ciprini , Gino Tosti , Harri Teräsranta , Hugh D. Aller

Context. We present the light curves of six BL Lac objects, PKS 0537-441, PKS 0735+17, OJ 287, PKS 2005-489, PKS 2155-304, W Comae, and of the flat spectrum radio quasar PKS 1510-089, as a part of a photometric monitoring program in the…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Angela Sandrinelli , Stefano Covino , Aldo Treves

Context. QSO B1420+326 is a blazar classified as a Flat Spectrum Radio Quasar (FSRQ). In the beginning of 2020 it underwent an enhanced flux state. An extensive multiwavelength campaign allowed us to trace the evolution of the flare. Aims.…

High Energy Astrophysical Phenomena · Physics 2021-05-05 V. A. Acciari , S. Ansoldi , L. A. Antonelli , A. Arbet Engels , M. Artero , K. Asano , D. Baack , A. Babić , A. Baquero , U. Barres de Almeida , J. A. Barrio , J. Becerra González , W. Bednarek , L. Bellizzi , E. Bernardini , M. Bernardos , A. Berti , J. Besenrieder , W. Bhattacharyya , C. Bigongiari , A. Biland , O. Blanch , G. Bonnoli , Ž. Bošnjak , G. Busetto , R. Carosi , G. Ceribella , M. Cerruti , Y. Chai , A. Chilingarian , S. Cikota , S. M. Colak , E. Colombo , J. L. Contreras , J. Cortina , S. Covino , G. D'Amico , V. D'Elia , P. Da Vela , F. Dazzi , A. De Angelis , B. De Lotto , M. Delfino , J. Delgado , C. Delgado Mendez , D. Depaoli , F. Di Pierro , L. Di Venere , E. Do Souto Espiñeira , D. Dominis Prester , A. Donini , D. Dorner , M. Doro , D. Elsaesser , V. Fallah Ramazani , A. Fattorini , G. Ferrara , L. Foffano , M. V. Fonseca , L. Font , C. Fruck , S. Fukami , R. J. García López , M. Garczarczyk , S. Gasparyan , M. Gaug , N. Giglietto , F. Giordano , P. Gliwny , N. Godinović , J. G. Green , D. Green , D. Hadasch , A. Hahn , L. Heckmann , J. Herrera , J. Hoang , D. Hrupec , M. Hütten , T. Inada , S. Inoue , K. Ishio , Y. Iwamura , J. Jormanainen , L. Jouvin , Y. Kajiwara , M. Karjalainen , D. Kerszberg , Y. Kobayashi , H. Kubo , J. Kushida , A. Lamastra , D. Lelas , F. Leone , E. Lindfors , S. Lombardi , F. Longo , R. López-Coto , M. López-Moya , A. López-Oramas , S. Loporchio , B. Machado de Oliveira Fraga , C. Maggio , P. Majumdar , M. Makariev , M. Mallamaci , G. Maneva , M. Manganaro , K. Mannheim , L. Maraschi , M. Mariotti , M. Martínez , D. Mazin , S. Mender , S. Mićanović , D. Miceli , T. Miener , M. Minev , J. M. Miranda , R. Mirzoyan , E. Molina , A. Moralejo , D. Morcuende , V. Moreno , E. Moretti , V. Neustroev , C. Nigro , K. Nilsson , D. Ninci , K. Nishijima , K. Noda , S. Nozaki , Y. Ohtani , T. Oka , J. Otero-Santos , S. Paiano , M. Palatiello , D. Paneque , R. Paoletti , J. M. Paredes , L. Pavletić , P. Peñil , C. Perennes , M. Persic , P. G. Prada Moroni , E. Prandini , C. Priyadarshi , I. Puljak , W. Rhode , M. Ribó , J. Rico , C. Righi , A. Rugliancich , L. Saha , N. Sahakyan , T. Saito , S. Sakurai , K. Satalecka , F. G. Saturni , B. Schleicher , K. Schmidt , T. Schweizer , J. Sitarek , I. Šnidarić , D. Sobczynska , A. Spolon , A. Stamerra , D. Strom , M. Strzys , Y. Suda , T. Surić , M. Takahashi , F. Tavecchio , P. Temnikov , T. Terzić , M. Teshima , N. Torres-Albà , L. Tosti , S. Truzzi , A. Tutone , J. van Scherpenberg , G. Vanzo , M. Vazquez Acosta , S. Ventura , V. Verguilov , C. F. Vigorito , V. Vitale , I. Vovk , M. Will , D. Zarić , R. Angioni , F. D'Ammando , S. Ciprini , C. C. Cheung , M. Orienti , L. Pacciani , P. Prajapati , P. Kumar , S. Ganesh , M. Minev , A. Kurtenkov , A. Marchini , L. Carrasco , G. Escobedo , A. Porras , E. Recillas , A. Lähteenmäki , M. Tornikoski , M. Berton , J. Tammi , R. J. C. Vera , S. G. Jorstad , A. P. Marscher , Z. R. Weaver , M. Hart , M. K. Hallum , V. M. Larionov , G. A. Borman , T. S. Grishina , E. N. Kopatskaya , E. G. Larionova , A. A. Nikiforova , D. A. Morozova , S. S. Savchenko , Yu. V. Troitskaya , I. S. Troitsky , A. A. Vasilyev , M. Hodges , T. Hovatta , S. Kiehlmann , W. Max-Moerbeck , A. C. S. Readhead , R. Reeves , T. J. Pearson
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