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Related papers: BL Lac candidates for TeV observations

200 papers

The EGRET instrument on the Compton Gamma Ray Observatory (1991-2000) has positively detected high energy gamma-ray emission from more than 67 active galaxies of the blazar class. The majority of the EGRET blazars are flat-spectrum radio…

Astrophysics · Physics 2009-11-06 R. Mukherjee

A sample of 54 selected Active Galactic Nuclei (AGN) has been observed with the HEGRA stereoscopic system of Cherenkov Telescopes between 1996 and 2002 in the TeV energy regime. The observations were motivated by the positive results…

Astrophysics · Physics 2018-01-31 The HEGRA Collaboration , F. Aharonian , A. Akhperjanian , M. Beilicke

Large-scale extragalactic jets, observed to extend from a few to a few hundred kiloparsecs from active galactic nuclei, are now studied over many decades in frequency of electromagnetic spectrum, from radio until (possibly) TeV gamma rays.…

Astrophysics · Physics 2017-11-01 L. Stawarz

A set of potentially gamma-ray--loud BL Lac objects is selected by intersecting the EGRET and BL Lac catalogs. Of the resulting 14 objects, eight are found to correlate with arrival directions of ultra--high-energy cosmic rays (UHECRs),…

Astrophysics · Physics 2009-11-07 D. Gorbunov , P. Tinyakov , I. Tkachev , S. Troitsky

Context. Star-forming galaxies emit {\gamma}rays with relatively low luminosity, but the study of their emission is no less captivating. While it is known that their {\gamma}-ray luminosity in the GeV band is strongly linked to their star…

High Energy Astrophysical Phenomena · Physics 2025-07-02 P. Kornecki , J. Biteau , C. Boisson , P. Cristofari

We performed an observational program with the X-ray satellite BeppoSAX to study objects with extreme synchrotron peak frequencies (nu_peak > 1 keV). Of the seven sources observed, four showed peak frequencies in the range 1-5 keV, while…

In an attempt to increase the number of known microquasars, Paredes et al. (2002) have presented a long-term project focused on the search for new objects of this type. They performed a cross-identification between X-ray and radio catalogs…

Astrophysics · Physics 2007-05-23 M. Ribo , E. Ros , J. M. Paredes , M. Massi , J. Marti

We utilize machine learning methods to distinguish BL Lacertae objects (BL Lac) from Flat Spectrum Radio Quasars (FSRQ) within a sample of likely X-ray blazar counterparts to Fermi 3FGL unassociated gamma-ray sources. From our previous…

High Energy Astrophysical Phenomena · Physics 2021-03-03 Amanpreet Kaur , Abraham D. Falcone , Michael C. Stroh

In recent years, the number of known sources emitting very- and ultra-high-energy gamma-rays has increased significantly thanks to facilities such as LHAASO and HAWC. Many of the observed sources are still unidentified or poorly constrained…

High Energy Astrophysical Phenomena · Physics 2025-09-19 Michela Rigoselli , Sarah Recchia , Alberto Bonollo , Silvia Crestan , Giada Peron , Andrea Giuliani , Sandro Mereghetti

The wealth of recent data from imaging air Cherenkov telescopes (IACTs), ultra-high energy cosmic-ray experiments and neutrino telescopes have fuelled a renewed interest in hadronic emission models for gamma-loud blazars. We explore…

High Energy Astrophysical Phenomena · Physics 2017-06-08 Andreas Zech , Matteo Cerruti , Daniel Mazin

We analyse 77 \textit{Fermi} sources and their potential low-energy counterparts previously proposed in the literature. These sources were classified as active galactic nuclei, mainly blazars, based on optical spectroscopy. The main goals…

High Energy Astrophysical Phenomena · Physics 2025-09-03 Alberto Ulgiati , Paolo Padovani , Paolo Giommi , Simona Paiano , Ciro Pinto

We report on optical searches in the error circles of 93 ROSAT survey sources located at low galactic latitudes (|b| < 20 deg). These sources were extracted from the ROSAT Galactic Plane Survey using various selection criteria on hardness…

Multi-wavelength observations with TeV photons are an essential diagnostic tool to study the physics of TeV sources. The complex variability of blazars, however (timescales from years down to minutes, with different patterns and SED…

Astrophysics · Physics 2009-11-10 L. Costamante

We study the cosmological evolution of BL Lac objects by applying the Ve/Va analysis to a new sample of 55 objects presented for the first time in this paper. This sample has been selected from the 239 sources with the brightest X-ray flux…

Astrophysics · Physics 2009-11-07 A. Caccianiga , T. Maccacaro , A. Wolter , R. Della Ceca , I. M. Gioia

AIMS. We are studying an unbiased sample of 42 nearby (z < 0.2) BL Lacertae objects with a multi-wavelength approach. The results of VLBI observations were presented in the first paper of this series. In this paper, we study the…

High Energy Astrophysical Phenomena · Physics 2018-11-08 F. D'Ammando , M. Giroletti , S. Rainò

Based on identifications from the Veron and Quasars.org catalogs, we determine the optical-to-X-ray spectral indices for a sample of 201 BL Lac type objects (BLLs) and search for trends in the distribution of these indices of the sources…

Astrophysics · Physics 2009-11-13 Sergey Troitsky

This talk focuses on the statistical properties of X-ray selected BL Lacertae objects (XBLs) whose catalogue has been compiled. It consists of 312 sources from different X-ray surveys, unambiguously identified to mid-2010. Results of the…

Cosmology and Nongalactic Astrophysics · Physics 2011-11-03 B. Z. Kapanadze

Recent Cerenkov observations of the two BL Lac objects PKS 2155-304 and Mkn 501 revealed TeV flux variability by a factor ~2 in just 3-5 minutes. Even accounting for the effects of relativistic beaming, such short timescales are challenging…

Astrophysics · Physics 2009-11-13 G. Ghisellini , F. Tavecchio , G. Bodo , A. Celotti

Although blazars are thought to emit most of their luminosity in the gamma-ray band, there are subclasses of them very prominent in hard X-rays. These are the best candidates to be studied by Simbol-X. They are at the extremes of the blazar…

Cosmology and Nongalactic Astrophysics · Physics 2009-06-25 Gabriele Ghisellini

The extragalactic background light (EBL), the cumulative radiation from all extragalactic sources, traces galaxy formation and cosmic evolution. High-energy $\gamma$ rays attenuated via pair production with EBL photons are a powerful probe…

High Energy Astrophysical Phenomena · Physics 2026-04-13 J. Baxter , A. Dominguez , J. D. Finke , A. Desai , M. Ajello , A. Banerjee , Dieter Hartmann , Vaidehi S. Paliya