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Previously suggested correlations of BL Lac type objects with the arrival directions of the ultra-high-energy cosmic ray primaries are tested by making use of the HiRes stereoscopic data. The results of the study support the conclusion that…

Astrophysics · Physics 2008-11-26 D. S. Gorbunov , P. G. Tinyakov , I. I. Tkachev , S. V. Troitsky

We report results from {\it XMM-Newton} observations of thirteen X-ray bright BL Lacertae objects, selected from the {\it Einstein} Slew Survey sample. The spectra are generally well fit by power-law models, with four objects having hard…

The large majority of BL Lacertae objects belonging to the 1 Jy sample, the class prototype for radio-selected sources, are thought to emit most of their synchrotron power in the far IR band. Ironically, this spectral region is very…

Astrophysics · Physics 2007-05-23 P. Padovani , P. Giommi , P. Abraham , S. Csizmadia , A. Moor

The variability of the high-frequency peaked BL Lac object PKS 2155-304 is studied using almost 10 years of optical, X-ray and gamma-rays data. Publicly available data have been gathered and analyzed with the aim to characterize the…

High Energy Astrophysical Phenomena · Physics 2019-01-16 J. Chevalier , D. A. Sanchez , P. D. Serpico , J. -P. Lenain , G. Maurin

We present new clues to the problem of the radio loudness dichotomy arising from an extensive search for intranight optical variability in seven sets of optically luminous radio-quiet quasars and (radio-loud) BL Lacertae objects, which are…

Astrophysics · Physics 2009-11-07 Gopal-Krishna , C. S. Stalin , Ram Sagar , Paul J. Wiita

Gigahertz Peaked Spectrum (GPS) sources and Compact Symmetric Objects (CSO) are selected in very different ways, but have a significant overlap in properties. Ever since their discovery it has been speculated that they are young objects,…

Astrophysics · Physics 2007-05-23 Ignas Snellen , Richard Schilizzi

We propose a new physical model for the unification of all Blazars. The blazar phenomenology can be accounted for by a sequence in the source power and intensity of the diffuse radiation field surrounding the relativistic jet. This…

Astrophysics · Physics 2007-05-23 G. Fossati

We calculate the spectral energy distribution (SED) of electromagnetic radiation and the spectrum of high energy neutrinos from BL Lac objects in the context of the Synchrotron Proton Blazar Model. In this model, the high energy hump of the…

Astrophysics · Physics 2008-11-26 A. Muecke , R. J. Protheroe , R. Engel , J. P. Rachen , T. Stanev

In this paper we compile the analysis of ~ 200 synchrotron flare events from ~ 90 distinct objects/events for which the distance is well established, and hence the peak luminosity can be accurately estimated. For each event we measure this…

High Energy Astrophysical Phenomena · Physics 2015-06-23 M. Pietka , R. P. Fender , E. F. Keane

Near--infrared, optical and ultraviolet quasi--simultaneous observations of 11 BL Lacertae objects are reported. For all but one source the dereddened spectral flux distribution in the $8\cdot10^{13}-2\cdot10^{15}$ Hz frequency range can be…

Astrophysics · Physics 2009-10-22 E. Pian , R. Falomo , R. Scarpa , A. Treves

BL Lacertae is a blazar known for its high flux variability and occasional broadband flares of unknown origin. It was in an extended flaring state from July 2020 until the end of 2021, making it an ideal candidate to study spectral and…

High Energy Astrophysical Phenomena · Physics 2026-04-01 A. Priyana Noel , Alicja Wierzcholska , Raj Prince

We present simultaneous multifrequency radio observations for a complete subsample of 26 XBLs from the Einstein Extended Medium-Sensitivity Survey, obtained with the Very Large Array (VLA). Spectra are computed using fluxes at 20, 6 and 3.6…

Astrophysics · Physics 2009-11-10 Francesca Cavallotti , Anna Wolter , John T. Stocke , Travis Rector

We examine the potential multi-messenger role of BL Lac objects emitting at high energy (so-called HBL) focusing on the limits on the energy density of soft radiation in the jet frame, a critical parameter which regulates the proton cooling…

High Energy Astrophysical Phenomena · Physics 2019-07-24 F. Tavecchio , F. Oikonomou , C. Righi

Blazars are characterized by large amplitude and fast variability, indicating that the electron distribution is rapidly changing, often on time scales shorter than the light crossing time. The emitting region is sufficiently compact to let…

Astrophysics · Physics 2009-10-31 Marco Chiaberge , Gabriele Ghisellini

Blazars are characterized by large amplitude and fast variability, indicating that the electron distribution is rapidly changing, often on time scales shorter than the light crossing time. We study the time dependent behavior of the…

Astrophysics · Physics 2007-05-23 Marco Chiaberge , Gabriele Ghisellini

We construct the first X-ray selected sample of radio-loud quasars from the EMSS survey. The X-ray selection allows us to explore the properties of radio-loud quasars 10-100 weaker than classical samples in the radio band. There are no…

Astrophysics · Physics 2007-05-23 Anna Wolter , Annalisa Celotti

We present and discuss polarimetric observations of 182 targets drawn from an optically selected sample of 240 probable BL Lac candidates out of the SDSS compiled by Collinge et al. (2005). In contrast to most other BL Lac candidate samples…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 J. Heidt , K. Nilsson

We present new radio observations of 9 members of a sample of 29 nearby (z < 0.2) BL Lac objects. The new data have been obtained with the European VLBI Network and/or the MERLIN at 1.6 and 5 GHz and complement previous observations. For…

Astrophysics · Physics 2008-11-26 M. Giroletti , G. Giovannini , G. B. Taylor , R. Falomo

In the framework of the unification scheme of radio-loud active galactic nuclei, BL Lac objects and quasars are the beamed end-on counterparts of low-power (FRI) and high-power (FRII) radio galaxies, respectively. Some BL Lacs have been…

Astrophysics of Galaxies · Physics 2015-06-18 Natalia Zywucka , Arti Goyal , Marek Jamrozy , Michal Ostrowski , Lukasz Stawarz

Previous observational studies of the infrared (IR)-radio relation out to high redshift employed any detectable star forming systems at a given redshift within the restricted area of cosmological survey fields. Consequently, the evolution…