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BL Lac objects can be extreme in two ways: with their synchrotron emission, peaking beyond 1 keV in their spectral energy distribution, or with their gamma-ray emission, peaking at multi-TeV energies up to and beyond 10-20 TeV, like 1ES…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Luigi Costamante

Light curves of eight BL Lac objects in the BVRI bands have been analyzed. All of the objects tend to be bluer when brighter. However spectral slope changes differ quantitatively from those of a sample of QSOs analyzed in a previous paper…

Astrophysics · Physics 2009-11-07 Fausto Vagnetti , Dario Trevese , Roberto Nesci

Among active galactic nuclei, BL Lac objects show extreme properties that have been interpreted as the effect of relativistic beaming on the emission from a plasma jet oriented close to the line of sight. The Doppler amplification of the…

Astrophysics of Galaxies · Physics 2015-06-29 Alessandro Capetti , Claudia M. Raiteri

We present recent X-ray observations of intermediate BL Lac objects (IBLs), i.e. BL Lacs which are located between high-energy and low-energy peaked BL Lac objects with respect to alpha_rx. We briefly discuss the statistical properties of…

Astrophysics · Physics 2007-05-23 J. Siebert , W. Brinkmann , S. A. Laurent-Muehleisen , M. Matsuoka

We have organized an extensive multiwavelength campaign on BL Lacertae in the second half of 2000. Simultaneous or quasi-simultaneous observations were taken at radio frequencies, in the optical - carried out by the WEBT collaboration -, in…

We present a new sample of 30 nearby (z<0.2) BL Lacs, selected to study the nuclear as well as the large scale properties of low power radio sources. In this first paper, we show and discuss new radio data taken with the VLA (19 objects at…

Astrophysics · Physics 2009-11-10 M. Giroletti , G. Giovannini , G. B. Taylor , R. Falomo

The blazar sequence is reflected in a correlation of the peak luminosity versus peak frequency of the synchrotron component of blazars. This correlation has been considered one of the fundamental pieces of evidence for the existence of a…

High Energy Astrophysical Phenomena · Physics 2013-01-28 Justin D. Finke

We study the variability properties at radio frequencies of the jets thought to be typical of Active Galactic Nuclei, i.e. bulk Lorentz factor \Gamma ~ 10, and incoherent synchrotron emission. We assume that the radiating electrons are…

Astrophysics · Physics 2009-10-30 M. Spada , M. Salvati , F. Pacini

We present radio observations at three frequencies and contemporaneous optical monitoring of the peculiar BL Lac object AO 0235+164. During a three-week campaign with the VLA we observed intraday variability in this source and found a…

We present the results of extensive multi-band intra-night optical monitoring of BL Lacertae during 2010--2012. BL Lacertae was very active in this period and showed intense variability in almost all wavelengths. We extensively observed it…

BL Lacertae is the prototype of the BL Lac class of active galactic nuclei, exhibiting intensive activity on parsec (pc) scales, such as intense core variability and multiple ejections of jet components. In particular, in previous works the…

High Energy Astrophysical Phenomena · Physics 2015-06-11 Anderson Caproni , Zulema Abraham , Hektor Monteiro

We estimate the intrinsic luminosities and synchrotron peak frequency using the derived Doppler factor for a sample of 170 BL Lac objects, of which the synchrotron peak frequency are derived by fitting the SED constructed with the collected…

Astrophysics · Physics 2009-11-13 Zhongzu Wu , Minfeng Gu , D. R. Jiang

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

Blazars are a class of jet-dominated active galactic nuclei with a typical double-humped spectral energy distribution. It is of common consensus the Synchrotron emission to be responsible for the low frequency peak, while the origin of the…

High Energy Astrophysical Phenomena · Physics 2023-05-22 Riccardo Middei , Ioannis Liodakis , Matteo Perri , Simonetta Puccetti , Elisabetta Cavazzuti , Laura Di Gesu , Steven R. Ehlert , Grzegorz Madejski , Alan P. Marscher , Herman L. Marshall , Fabio Muleri , Michela Negro , Svetlana G. Jorstad , Beatriz Agís-González , Iván Agudo , Giacomo Bonnoli , Maria I. Bernardos , Víctor Casanova , Maya García-Comas , César Husillos , Alessandro Marchini , Alfredo Sota , Pouya M. Kouch , George A. Borman , Evgenia N. Kopatskaya , Elena G. Larionova , Daria A. Morozova , Sergey S. Savchenko , Andrey A. Vasilyev , Alexey V. Zhovtan , Carolina Casadio , Juan Escudero , Ioannis Myserlis , Antonio Hales , Seiji Kameno , Ruediger Kneissl , Hugo Messias , Hiroshi Nagai , Dmitry Blinov , Ioakeim G. Bourbah , Sebastian Kiehlmann , Evangelos Kontopodis , Nikos Mandarakas , Stylianos Romanopoulos , Raphael Skalidis , Anna Vervelaki , Joseph R. Masiero , Dimitri Mawet , Maxwell A. Millar-Blanchaer , Georgia V. Panopoulou , Samaporn Tinyanont , Andrei V. Berdyugin , Masato Kagitani , Vadim Kravtsov , Takeshi Sakanoi , Ryo Imazawa , Mahito Sasada , Yasushi Fukazawa , Koji S. Kawabata , Makoto Uemura , Tsunefumi Mizuno , Tatsuya Nakaoka , Hiroshi Akitaya , Mark Gurwell , Ramprasad Rao , Niccoló Di Lalla , Nicoló Cibrario , Immacolata Donnarumma , Dawoon E. Kim , Nicola Omodei , Luigi Pacciani , Juri Poutanen , Fabrizio Tavecchio , Lucio A. Antonelli , Matteo Bachetti , Luca Baldini , Wayne H. Baumgartner , Ronaldo Bellazzini , Stefano Bianchi , Stephen D. Bongiorno , Raffaella Bonino , Alessandro Brez , Niccoló Bucciantini , Fiamma Capitanio , Simone Castellano , Stefano Ciprini , Enrico Costa , Alessandra De Rosa , Ettore Del Monte , Alessandro Di Marco , Victor Doroshenko , Michal Dovčiak , Teruaki Enoto , Yuri Evangelista , Sergio Fabiani , Riccardo Ferrazzoli , Javier A. Garcia , Shuichi Gunji , Kiyoshi Hayashida , Jeremy Heyl , Wataru Iwakiri , Vladimir Karas , Takao Kitaguchi , Jeffery J. Kolodziejczak , Henric Krawczynski , Fabio La Monaca , Luca Latronico , Simone Maldera , Alberto Manfreda , Frédéric Marin , Andrea Marinucci , Francesco Massaro , Giorgio Matt , Ikuyuki Mitsuishi , C. -Y. Ng , Stephen L. O'Dell , Chiara Oppedisano , Alessandro Papitto , George G. Pavlov , Abel L. Peirson , Melissa Pesce-Rollins , Pierre-Olivier Petrucci , Maura Pilia , Andrea Possenti , Brian D. Ramsey , John Rankin , Ajay Ratheesh , Roger W. Romani , Carmelo Sgró , Patrick Slane , Paolo Soffitta , Gloria Spandre , Toru Tamagawa , Roberto Taverna , Yuzuru Tawara , Allyn F. Tennant , Nicholas E. Thomas , Francesco Tombesi , Alessio Trois , Sergey Tsygankov , Roberto Turolla , Jacco Vink , Martin C. Weisskopf , Kinwah Wu , Fei Xie , Silvia Zane

The recent Cherenkov telescope observations and detections of the BL Lac objects Mkn 421, Mkn 501, 1ES 2344+514, PKS 2155--304 and possibly 1ES 1959+658 have shown that there exists a subclass of BL Lac objects emitting a substantial…

Astrophysics · Physics 2009-10-31 Gabriele Ghisellini

We introduce a new method to determine the redshift of unknown-redshift BL Lac Objects. The method relies on simultaneous multi-wavelength (MWL) observations of BL Lac objects in optical, X-ray, HE (E>100 MeV) gamma-rays and VHE (E>100…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Nijil Mankuzhiyil , Stefano Ansoldi , Gessica De Caneva , Massimo Persic , Fabrizio Tavecchio

After a brief critical overview of the main properties of blazars and their classification, some significant results from recent multiwavelength observations are summarized, in the context of the jet physics.

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 L. Costamante

The possibility to detect simultaneously in the X-ray band the synchrotron and Inverse Compton (IC)emission of intermediate BL Lac objects offers the unique opportunity to study contemporaneously the low- and high-energy tails of the…

Astrophysics · Physics 2009-11-11 E. Ferrero , S. J. Wagner , D. Emmanoulopoulos , L. Ostorero

The recent BeppoSAX observations of the BL Lac objects Mkn 501 and 1ES 2344+514 have shown that the synchrotron spectrum of these objects peaks, in a v-vF(v) representation, at energies at or above 100 keV. One can wonder if these are the…

Astrophysics · Physics 2007-05-23 Gabriele Ghisellini

The results of VLBI total intensity (I) and linear polarization (P) observations at 6cm are presented for ten radio bright BL Lacertae objects. These images complete first-epoch polarization observations for the 1-Jy sample of northern BL…

Astrophysics · Physics 2009-11-10 D. C. Gabuzda , A. B. Pushkarev , T. V. Cawthorne