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The BL Lac object S5~0716+714, a highly variable blazar, underwent an impressive outburst in January 2015 (Phase A), followed by minor activity in February (Phase B). The MAGIC observations were triggered by the optical flux observed in…

High Energy Astrophysical Phenomena · Physics 2020-01-29 MAGIC Collaboration , M. L. Ahnen , S. Ansoldi , L. A. Antonelli , C. Arcaro , D. Baack , A. Babić , B. Banerjee , P. Bangale , U. Barres de Almeida , J. A. Barrio , J. Becerra González , W. Bednarek , E. Bernardini , R. Ch. Berse , A. Berti , W. Bhattacharyya , A. Biland , O. Blanch , G. Bonnoli , R. Carosi , A. Carosi , G. Ceribella , A. Chatterjee , S. M. Colak , P. Colin , E. Colombo , J. L. Contreras , J. Cortina , S. Covino , P. Cumani , P. Da Vela , F. Dazzi , A. De Angelis , B. De Lotto , M. Delfino , J. Delgado , F. Di Pierro , A. Domínguez , D. Dominis Prester , D. Dorner , M. Doro , S. Einecke , D. Elsaesser , V. Fallah Ramazani , A. Fernández-Barral , D. Fidalgo , M. V. Fonseca , L. Font , C. Fruck , D. Galindo , S. Gallozzi , R. J. García López , M. Garczarczyk , M. Gaug , P. Giammaria , N. Godinović , D. Gora , D. Guberman , D. Hadasch , A. Hahn , T. Hassan , M. Hayashida , J. Herrera , J. Hose , D. Hrupec , K. Ishio , Y. Konno , H. Kubo , J. Kushida , D. Kuveždić , D. Lelas , E. Lindfors , S. Lombardi , F. Longo , M. López , C. Maggio , P. Majumdar , M. Makariev , G. Maneva , M. Manganaro , K. Mannheim , L. Maraschi , M. Mariotti , M. Martínez , S. Masuda , D. Mazin , K. Mielke , M. Minev , J. M. Miranda , R. Mirzoyan , A. Moralejo , V. Moreno , E. Moretti , T. Nagayoshi , V. Neustroev , A. Niedzwiecki , M. Nievas Rosillo , C. Nigro , K. Nilsson , D. Ninci , K. Nishijima , K. Noda , L. Nogués , S. Paiano , J. Palacio , D. Paneque , R. Paoletti , J. M. Paredes , G. Pedaletti , M. Peresano , M. Persic , P. G. Prada Moroni , E. Prandini , I. Puljak , J. R. Garcia , I. Reichardt , W. Rhode , M. Ribó , J. Rico , C. Righi , A. Rugliancich , T. Saito , K. Satalecka , T. Schweizer , J. Sitarek , I. Šnidarić , D. Sobczynska , A. Stamerra , M. Strzys , T. Surić , M. Takahashi , L. Takalo , F. Tavecchio , P. Temnikov , T. Terzić , M. Teshima , N. Torres-Albà , A. Treves , S. Tsujimoto , G. Vanzo , M. Vazquez Acosta , I. Vovk , J. E. Ward , M. Will , D. Zarić , Fermi-LAT Collaboration , D. Bastieri , D. Gasparrini , B. Lott , B. Rani , D. J. Thompson , MWL Collaborators , I. Agudo , E. Angelakis , G. A. Borman , C. Casadio , T. S. Grishina , M. Gurwell , T. Hovatta , R. Itoh , E. Järvelä , H. Jermak , S. Jorstad , E. N. Kopatskaya , A. Kraus , T. P. Krichbaum , N. P. M. Kuin , A. Lähteenmäki , V. M. Larionov , L. V. Larionova , A. Y. Lien , G. Madejski , A. Marscher , I. Myserlis , W. Max-Moerbeck , S. N. Molina , D. A. Morozova , K. Nalewajko , T. J. Pearson , V. Ramakrishnan , A. C. S. Readhead , R. A. Reeves , S. S. Savchenko , I. A. Steele , M. Tornikoski , Yu. V. Troitskaya , I. Troitsky , A. A. Vasilyev , J. Anton Zensus

The source CGRaBS~J0211$+$1051 (MG1 J021114+1051, z=0.20) flared up on 2011 January 23 in high-energy $\gamma$-rays as reported by {\it Fermi}/LAT. This event was followed by the increased activity at the UV, optical and radio frequencies…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Sunil Chandra , Kiran S Baliyan , Shashikiran Ganesh , Luigi Foschini

The unification of X-ray and radio selected BL Lacs has been an outstanding problem in the blazar research in the past years. Recent investigations have shown that the gap between the two classes can be filled with intermediate objects and…

Astrophysics · Physics 2011-05-23 V. Beckmann , D. Engels , N. Bade , O. Wucknitz

We selected a sample of 437 BL Lac objects, taken from the RomaBZCat catalogue, for which spectroscopic information and SDSS photometry is available. We propose a new classification of BL Lacs in which the sources' type is not defined only…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Enrico Massaro , Roberto Nesci , Silvia Piranomonte

BL Lacertae (BL Lac) objects at high redshifts ($z\geq 2$) are rarely detected. Through careful analysis of the SDSS spectrum, BZB J1450+5201 is confirmed to be a high-$z$ BL Lac object with $z\geq$ 2.471 by identifying the Ly$\alpha$ 1216…

High Energy Astrophysical Phenomena · Physics 2016-03-23 N. H. Liao , J. M. Bai , J. G. Wang , H. T. Liu , J. J. Zhang , Ning Jiang , Z. L. Yuan , Liang Chen

The determination of the redshift of extragalactic gamma ray sources is of fundamental importance for the interpretation of their emission models and extragalactic population studies, AGN classification schemes, and to study the interaction…

Astrophysics of Galaxies · Physics 2016-03-16 Simona Paiano , Marco Landoni , Renato Falomo , Riccardo Scarpa , Aldo Treves

Extreme high-frequency peaked BL Lacs (EHBLs) are characterized by a synchrotron peak frequency exceeding $10^{17}$ Hz and a second peak that can be in the energy range of few GeVs to several TeVs. The MAGIC telescopes detected multi-TeV…

High Energy Astrophysical Phenomena · Physics 2023-01-10 B. Medina-Carrillo , Sarira Sahu , G. Sánchez-Colón , Subhash Rajpoot

Aims: The determination of elusive redshifts of bright BL Lac objects Methods: We use the capabilities of newly available spectrograph X-Shooter at European Southern Observatory (ESO) Very Large Telescope, that combines high resolution and…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Marco Landoni , Renato Falomo , Aldo Treves , Boris Sbarufatti , Roberto Decarli , Fabrizio Tavecchio , Jari Kotilainen

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 investigate the potential existence of a new population of BL Lacs, called ultra extreme high-energy-peaked BL Lacs (UEHBLs), whose synchrotron emission component peaks in the MeV band, extending the blazar sequence beyond its current…

High Energy Astrophysical Phenomena · Physics 2025-11-13 A. Sciaccaluga , F. Tavecchio , T. Sbarrato , G. Bonnoli

We propose a scenario where blazars are classified as flat-spectrum radio quasars (FSRQs), BL Lacs, low synchrotron, or high synchrotron peaked objects according to a varying mix of the Doppler boosted radiation from the jet, the emission…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 P. Giommi , P. Padovani , G. Polenta , S. Turriziani , V. D'Elia , S. Piranomonte

With their rapid, violent variability and broad featureless continuum emission, blazars have puzzled astronomers for over two decades. Today blazars represent the only extragalactic objects detected in high-energy gamma-rays. Their spectral…

Astrophysics · Physics 2009-10-31 Eric S. Perlman

We present coordinated multiwavelength observations of the bright, nearby BL Lac object Mrk 421 taken in 2013 January-March, involving GASP-WEBT, Swift, NuSTAR, Fermi-LAT, MAGIC, VERITAS, and other collaborations and instruments, providing…

High Energy Astrophysical Phenomena · Physics 2017-08-30 M. Baloković , D. Paneque , G. Madejski , A. Furniss , J. Chiang , the NuSTAR team , : , M. Ajello , D. M. Alexander , D. Barret , R. Blandford , S. E. Boggs , F. E. Christensen , W. W. Craig , K. Forster , P. Giommi , B. W. Grefenstette , C. J. Hailey , F. A. Harrison , A. Hornstrup , T. Kitaguchi , J. E. Koglin , K. K. Madsen , P. H. Mao , H. Miyasaka , K. Mori , M. Perri , M. J. Pivovaroff , S. Puccetti , V. Rana , D. Stern , G. Tagliaferri , C. M. Urry , N. J. Westergaard , W. W. Zhang , A. Zoglauer , the VERITAS collaboration , : , S. Archambault , A. A. Archer , A. Barnacka , W. Benbow , R. Bird , J. Buckley , V. Bugaev , M. Cerruti , X. Chen , L. Ciupik , M. P. Connolly , W. Cui , H. J. Dickinson , J. Dumm , J. D. Eisch , A. Falcone , Q. Feng , J. P. Finley , H. Fleischhack , L. Fortson , S. Griffin , S. T. Griffiths , J. Grube , G. Gyuk , M. Huetten , N. Haakansson , J. Holder , T. B. Humensky , C. A. Johnson , P. Kaaret , M. Kertzman , Y. Khassen , D. Kieda , M. Krause , F. Krennrich , M. J. Lang , G. Maier , S. McArthur , K. Meagher , P. Moriarty , T. Nelson , D. Nieto , R. A. Ong , N. Park , M. Pohl , A. Popkow , E. Pueschel , P. T. Reynolds , G. T. Richards , E. Roache , M. Santander , G. H. Sembroski , K. Shahinyan , A. W. Smith , D. Staszak , I. Telezhinsky , N. W. Todd , J. V. Tucci , J. Tyler , S. Vincent , A. Weinstein , A. Wilhelm , D. A. Williams , B. Zitzer , the MAGIC collaboration , : , M. L. Ahnen , S. Ansoldi , L. A. Antonelli , P. Antoranz , A. Babic , B. Banerjee , P. Bangale , U. Barres de Almeida , J. Barrio , J. Becerra González , W. Bednarek , E. Bernardini , B. Biasuzzi , A. Biland , O. Blanch , S. Bonnefoy , G. Bonnoli , F. Borracci , T. Bretz , E. Carmona , A. Carosi , A. Chatterjee , R. Clavero , P. Colin , E. Colombo , J. L. Contreras , J. Cortina , S. Covino , P. Da Vela , F. Dazzi , A. de Angelis , B. De Lotto , E. D. de Oña Wilhelmi , C. Delgado Mendez , F. Di Pierro , D. Dominis Prester , D. Dorner , M. Doro , S. Einecke , D. Elsaesser , A. Fernández-Barral , D. Fidalgo , M. V. Fonseca , L. Font , K. Frantzen , C. Fruck , D. Galindo , R. J. García López , M. Garczarczyk , D. Garrido Terrats , M. Gaug , P. Giammaria , D. Eisenacher , N. Godinović , A. González Muñoz , D. Guberman , A. Hahn , Y. Hanabata , M. Hayashida , J. Herrera , J. Hose , D. Hrupec , G. Hughes , W. Idec , K. Kodani , Y. Konno , H. Kubo , J. Kushida , A. La Barbera , D. Lelas , E. Lindfors , S. Lombardi , F. Longo , M. López , R. López-Coto , A. López-Oramas , E. Lorenz , P. Majumdar , M. Makariev , K. Mallot , G. Maneva , M. Manganaro , K. Mannheim , L. Maraschi , B. Marcote , M. Mariotti , M. Martínez , D. Mazin , U. Menzel , J. M. Miranda , R. Mirzoyan , A. Moralejo , E. Moretti , D. Nakajima , V. Neustroev , A. Niedzwiecki , M. Nievas-Rosillo , K. Nilsson , K. Nishijima , K. Noda , R. Orito , A. Overkemping , S. Paiano , S. Palacio , M. Palatiello , R. Paoletti , J. M. Paredes , X. Paredes-Fortuny , M. Persic , J. Poutanen , P. G. Prada Moroni , E. Prandini , I. Puljak , W. Rhode , M. Ribó , J. Rico , J. Rodriguez Garcia , T. Saito , K. Satalecka , V. Scapin , C. Schultz , T. Schweizer , S. N. Shore , A. Sillanpää , J. Sitarek , I. Snidaric , D. Sobczynska , A. Stamerra , T. Steinbring , M. Strzys , L. O. Takalo , H. Takami , F. Tavecchio , P. Temnikov , T. Terzić , D. Tescaro , M. Teshima , J. Thaele , D. F. Torres , T. Toyama , A. Treves , V. Verguilov , I. Vovk , J. E. Ward , M. Will , M. H. Wu , R. Zanin , external collaborators , : , J. Perkins , F. Verrecchia , C. Leto , M. Böttcher , M. Villata , C. M. Raiteri , J. A. Acosta-Pulido , R. Bachev , A. Berdyugin , D. A. Blinov , M. I. Carnerero , W. P. Chen , P. Chinchilla , G. Damljanovic , C. Eswaraiah , T. S. Grishina , S. Ibryamov , B. Jordan , S. G. Jorstad , M. Joshi , E. N. Kopatskaya , O. M. Kurtanidze , S. O. Kurtanidze , E. G. Larionova , L. V. Larionova , V. M. Larionov , G. Latev , H. C. Lin , A. P. Marscher , A. A. Mokrushina , D. A. Morozova , M. G. Nikolashvili , E. Semkov , A. Strigachev , Yu. V. Troitskaya , I. S. Troitsky , O. Vince , J. Barnes , T. Güver , J. W. Moody , A. C. Sadun , S. Sun , T. Hovatta , J. L. Richards , W. Max-Moerbeck , A. C. Readhead , A. Lähteenmäki , M. Tornikoski , J. Tammi , V. Ramakrishnan , R. Reinthal , E. Angelakis , L. Fuhrmann , I. Myserlis , V. Karamanavis , A. Sievers , H. Ungerechts , J. A. Zensus

Aims: The BL Lac object RGB J0152+017 (z=0.080) was predicted to be a very high-energy (VHE; > 100 GeV) gamma-ray source, due to its high X-ray and radio fluxes. Our aim is to understand the radiative processes by investigating the observed…

Astrophysics · Physics 2008-04-09 HESS Collaboration , F. Aharonian

Blazars are a peculiar class of active galactic nuclei (AGNs) that enlighten the sky at all wavelengths. The electromagnetic emission of these sources is jet-dominated resulting in a spectral energy distribution (SED) that has a typical…

High Energy Astrophysical Phenomena · Physics 2022-06-29 Riccardo Middei , Paolo Giommi , Matteo Perri , Sara Turriziani , Narek Sahakyan , Y. L. Chang , C. Leto , F. Verrecchia

The BL Lac object 4FGLJ0955.1+3551 has been suggested as a possible source of ultra energetic neutrinos detected by the Icecube observatory. The target was observed in January 2020 at the Large Binocular Telescope. Our spectroscopy…

High Energy Astrophysical Phenomena · Physics 2020-04-22 Simona Paiano , Renato Falomo , Paolo Padovani , Paolo Giommi , Adriana Gargiulo , Michela Uslenghi , Andrea Rossi , Aldo Treves

The Fermi Gamma-ray Observatory discovered about a thousand extragalactic sources emitting energy from 100 MeV to 100 GeV. The majority of these sources belong to the class of blazars characterized by a quasi-featureless optical spectrum…

Astrophysics of Galaxies · Physics 2017-11-02 Simona Paiano , Renato Falomo , Marco Landoni , Aldo Treves , Riccardo Scarpa

BL Lacertae (Lac) objects that are detected at very-high energies (VHE) are of fundamental importance to study multiple astrophysical processes, including the physics of jets, the properties of the extragalactic background light and the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Michele Fumagalli , Miroslava Dessauges-Zavadsky , Amy Furniss , J. Xavier Prochaska , David Williams , Kyle Kaplan , Matthew Hogan

Blazars are some of the brightest UV and X-ray sources in the sky and are valuable probes of the elusive warm-hot intergalactic medium (WHIM; $T{\simeq} 10^5-10^7$ K). However, many of the brightest blazars$-$called BL Lac objects such as…

Astrophysics of Galaxies · Physics 2021-12-15 J. Dorigo Jones , S. D. Johnson , Sowgat Muzahid , J. Charlton , H. -W. Chen , A. Narayanan , Sameer , J. Schaye , N. A. Wijers

All but three (M87, BL Lac and 3C 279) extragalactic sources detected so far at very high energy (VHE) gamma-rays belong to the class of high-frequency peaked BL Lac (HBL) objects. This suggested to us a systematic scan of candidate sources…

Astrophysics · Physics 2019-08-12 M. Meyer
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