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Related papers: The luminosity function of TeV-emitting BL Lacs: o…

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Over seventy blazars identified as sources of TeV gamma ray emission have been detected, including approximately sixty BL Lac objects and seven flat spectrum radio quasars. The distribution in space of these objects can be described by a…

High Energy Astrophysical Phenomena · Physics 2019-08-27 Aryeh Brill

BL Lacertae objects (BL Lacs) is the dominant population of TeV emitting blazars. In this work, we investigate whether there is any special observational properties for TeV sources. To do so, we will compare the observational properties of…

High Energy Astrophysical Phenomena · Physics 2016-07-13 C. Lin , J. H. Fan

Most of the ~50 blazars detected to date at TeV energies (E>0.1 TeV) are high-frequency-peaked BL Lacs (HBLs). Only a handful episodic TeV detections of low- and intermediate-frequency-peaked BL Lacs (LBL/IBLs, with synchrotron peak…

High Energy Astrophysical Phenomena · Physics 2019-08-13 M. Errando

Extreme high-energy peaked BL Lac objects (EHBLs) are an emerging class of blazars with exceptional spectral properties. The non-thermal emission of the relativistic jet peaks in the spectral energy distribution (SED) plot with the…

High Energy Astrophysical Phenomena · Physics 2019-07-19 L. Foffano , E. Prandini , A. Franceschini , S. Paiano

TeV-emitting BL Lac type blazars represent the extreme end of the blazar population. They are characterized by relatively weak jets and radiatively inefficient accretion disks. Particles accelerated in these jets experience fewer radiative…

High Energy Astrophysical Phenomena · Physics 2025-08-14 Cassidy Metzger , Andrea Gokus , Manel Errando

Extreme high-energy peaked BL Lac objects (EHBLs) are an emerging class of blazars with exceptional spectral properties. In blazars, the spectral energy distribution (SED) is dominated by the non-thermal emission of the relativistic jet,…

High Energy Astrophysical Phenomena · Physics 2019-07-31 L. Foffano , E. Prandini , A. Franceschini , S. Paiano

VERITAS is an array of four 12-m atmospheric Cherenkov telescopes, designed to observe the very-high-energy (VHE; E $\geq$100 GeV) sky. Since 2007, it has detected more than 20 extra-galactic sources, the majority of which are…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Matteo Cerruti

Here we present highlights from VERITAS observations of high-frequency-peaked BL Lac objects (HBLs). We discuss the key science motivations for observing these sources -- including performing multiwavelength campaigns critical to…

High Energy Astrophysical Phenomena · Physics 2019-08-13 M. Orr

We focus our analysis on 55 BL Lac objects with a hard Fermi gamma-ray spectrum, and for which a redshift or a lower limit to it has been determined by a previous study of ours. We extrapolate the spectral fits given by the 4FGL catalogue…

High Energy Astrophysical Phenomena · Physics 2021-10-20 Simona Paiano , Aldo Treves , Alberto Franceschini , Renato Falomo

Extremely High energy peaked BL Lac (EHBL) objects are a special class of blazars with peculiar observational properties at X-ray and $\gamma$--ray energies. The observations of these sources indicate hard X-ray and $\gamma$--ray spectra…

Astrophysics of Galaxies · Physics 2019-07-23 K K Singh , P J Meintjes , F A Ramamonjisoa , A Tolamatti

We report on our observations of the parsec-scale radio jet structures of five blazars that have been detected by ground-based TeV gamma-ray telescopes. These five blazars all belong to the class of high-frequency peaked BL Lac objects…

High Energy Astrophysical Phenomena · Physics 2012-05-14 Vivian C. Tiet , B. Glenn Piner , Philip G. Edwards

The VERITAS array of imaging atmospheric Cherenkov telescopes has collected nearly 6000 hours of observations of active galactic nuclei (AGNs). It has detected 39 very-high-energy (VHE, >100 GeV) AGNs at redshifts up to z = 0.9, of which 24…

High Energy Astrophysical Phenomena · Physics 2019-08-09 Orel Gueta

The HEGRA system of four Imaging Atmospheric Cherenkov Telescopes (IACTs) has been used to extensively observe extragalactic objects. In this paper we describe the search for TeV emission from nine very promising potential TeV sources,…

Astrophysics · Physics 2007-05-23 F. Aharonian , The HEGRA Collaboration

BL Lac objects detected at TeV energies preferentially belong to the subclass called 'high-frequency-peaked' BL Lacs (HBLs). Parsec-scale radio jets in these TeV-HBLs often show dominant, slow moving radio knots that are at most mildly…

High Energy Astrophysical Phenomena · Physics 2023-06-28 Vibhore Negi , Gopal-Krishna , Hum Chand , Silke Britzen

Most of the extragalactic sources detected at TeV energies are BL Lac objects. They belong to the subclass of "high frequency peaked BL Lacs" (HBLs) exhibiting spectral energy distributions with a lower energy peak in the X-ray band; this…

High Energy Astrophysical Phenomena · Physics 2015-06-04 F. Massaro , A. Paggi , M. Elvis , A. Cavaliere

Blazars are among the most energetic and violent objects in the universe. By observing blazars at very high energies (VHE, E > 100 GeV) we can better understand blazar emission mechanisms, jet structure, black hole accretion and the…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-13 J. S. Perkins

The VERITAS array of 12-m atmospheric-Cherenkov telescopes is used in an intensive observation program focused on the discovery of VHE (E > 100 GeV) gamma-ray-emitting blazars. Since VERITAS began full-scale operation in 2007, more than…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Wystan Benbow

The improved sensitivity of current-generation atmospheric-Cherenkov telescope (ACT) arrays enables us to probe for the first time low-frequency-peaked and intermediate-frequency-peaked BL Lac (LBL and IBL, respectively) objects as very…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Pratik Majumdar

The High Energy Stereoscopic System (H.E.S.S.) experiment, a ground-based gamma-ray Cherenkov telescope array located in Namibia, has now detected many extragalactic objects, which redshifts range from z=0.00183 up to z=0.2, possibly more.…

Astrophysics · Physics 2007-09-12 Jean-Philippe Lenain

The REX (Radio-Emitting X-ray sources) is a catalogue produced by cross-matching X-ray data from the ROSAT-PSPC archive of pointed observations and radio data from the NRAO VLA Sky Survey, aimed at the selection of blazars. From the REX…

High Energy Astrophysical Phenomena · Physics 2020-01-08 B. Balmaverde , A. Caccianiga , R. Della Ceca , A. Wolter , A. Belfiore , L. Ballo , M. Berton , I. Gioia , T. Maccacaro , B. Sbarufatti
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