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Related papers: New Extreme Synchrotron BL Lac Objects

200 papers

The multi-frequency `Sedentary Survey' is a deep, statistically complete, radio flux limited sample comprising 150 BL Lacertae objects distinguished by their extremely high X-ray to radio flux ratio, ranging from five hundred to over five…

Astrophysics · Physics 2007-05-23 P. Giommi , S. Piranomonte , M. Perri , P. Padovani

The BL Lac object 1ES 0229+200 (z=0.14) has been detected by HESS during observations taking place in 2005-2006. The TeV spectrum, when corrected for the absorption of gamma-ray photons through the interaction with the extragalactic…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 F. Tavecchio , G. Ghisellini , G. Ghirlanda , L. Costamante , A. Franceschini

Hard-TeV BL Lacs are a new type of blazars characterized by a hard intrinsic TeV spectrum, locating the peak of their gamma-ray emission in the spectral energy distribution (SED) above 2-10 TeV. Such high energies are problematic for the…

High Energy Astrophysical Phenomena · Physics 2018-05-16 L. Costamante , G. Bonnoli , F. Tavecchio , G. Ghisellini , G. Tagliaferri , D. Khangulyan

We present new BeppoSAX LECS, MECS, and PDS observations of four flat-spectrum radio quasars (FSRQ) having effective spectral indices alpha_ro and alpha_ox typical of high-energy peaked BL Lacs. Our sources have X-ray-to-radio flux ratios…

Astrophysics · Physics 2009-11-07 P. Padovani , L. Costamante , G. Ghisellini , P. Giommi , E. Perlman

A very high energy (VHE) gamma-ray signal has been detected at the 5.4 sigma level from H1426+428, an x-ray selected BL Lacertae object at a redshift of 0.129. The object was monitored from 1995 - 1998 with the Whipple 10m imaging…

Astrophysics · Physics 2019-08-14 D. Horan

The blazar 1ES 0229+200 is a high frequency peaked BL Lac object with a hard TeV spectrum extending to 10 TeV. Its unusual spectral characteristics make it a frequently used probe for intergalactic radiation and magnetic fields. With new,…

High Energy Astrophysical Phenomena · Physics 2015-05-30 S. Kaufmann , S. J. Wagner , O. Tibolla , M. Hauser

1ES1101-232 is a bright BL Lac of the High frequency peak class. We present here the results of two BeppoSAX observations in which the source has shown a variation of about 30% in flux with a corresponding spectral variability. We interpret…

Astrophysics · Physics 2007-05-23 A. Wolter , F. Tavecchio , A. Caccianiga , G. Ghisellini , G. Tagliaferri

The results of a BeppoSAX TOO observation of the BL Lac object Mkn421 during a high intensity state are reported and compared with monitoring X-ray data collected with the BeppoSAX Wide Field Cameras (WFC) and the RXTE All Sky Monitor(ASM).…

We present the results of a multi-wavelength study of a population of X-ray bright ($\rm log(F_{0.2-12 \ keV})>-12.5$), non-$\gamma$-ray detected high and extreme high synchrotron peak (HSP, EHSP; $\rm log(\nu_{\rm peak,\ Hz})>16$) BL Lacs…

High Energy Astrophysical Phenomena · Physics 2026-04-29 Federica Sibani , Stefano Marchesi , Ettore Bronzini , Marco Ajello , Michele Doro , Lea Marcotulli , Elisa Prandini , Cristian Vignali

Extremely high-peaked BL Lac objects (or extreme blazars) are unique extragalactic laboratories where particle acceleration processes are pushed at their physical limits. In these blazars, synchrotron emission peaking above keV energies is…

High Energy Astrophysical Phenomena · Physics 2025-10-08 L. Foffano , C. Arcaro , A. Arbet-Engels , F. D'Ammando , P. Da Vela , J. Jormanainen , D. Linder , S. Menon , E. Prandini , S. Ventura , E. Visentin

We report the multi-wavelength study for a high-synchrotron-peaked BL Lac 1ES 1218+304 using near-simultaneous data obtained during the period from January 1, 2018, to May 31, 2021 (MJD 58119-59365) from various instruments including…

High Energy Astrophysical Phenomena · Physics 2023-07-19 Rishank Diwan , Raj Prince , Aditi Agarwal , Debanjan Bose , Pratik Majumdar , Aykut Özdönmez , Sunil Chandra , Rukaiya Khatoon , Ergün Ege

We present new BeppoSAX LECS and MECS observations, covering the energy range 0.1 - 10 keV (observer's frame), of four BL Lacertae objects selected from the 1 Jy sample. All sources display a flat (alpha_x ~ 0.7) X-ray spectrum, which we…

Astrophysics · Physics 2009-11-10 P. Padovani , L. Costamante , P. Giommi , G. Ghisellini , A. Celotti , A. Wolter

We present X-ray spectra obtained with BeppoSAX (Satellite per Astronomia X) of 10 BL Lac objects, selected from the Einstein Medium Sensitivity and Slew Surveys. We find that in about half of the objects a fit in the 0.1-10 keV range with…

We summarize the results of BeppoSAX ToO observation of blazars that were known to be in a high state from observations carried out in the optical or X-ray or TeV bands.In some of the observed sources, two spectral components were detected,…

Astrophysics · Physics 2007-05-23 Gianpiero Tagliaferri , Gabriele Ghisellini , Marcello Ravasio

We present the preliminary results of a long BeppoSAX observation of the BL Lac object Mkn501 carried out in June 1999. The source was fainter than found during the BeppoSAX pointings of 1997 and 1998, but is still detected with a good…

We report on two BeppoSAX observations of BL Lac (2200+420) performed respectively in June and December 1999, as part of a ToO program to monitor blazars in high states of activity. During both runs the source has been detected up to 100…

PKS 2155-304 is one of the prototypes of BL Lac objects. Its spectral energy distribution is known from the radio to the TeV band and has two peaks, one in the soft X-rays and the other in the TeV region. These may be interpreted within the…

We present two BeppoSAX observations of BL Lac (2200+420) as part of a multiwavelength campaign performed in 2000. The source was in different states of activity: in June, the X-ray spectrum was faint and hard (alpha sim 0.8), with positive…

Astrophysics · Physics 2009-11-10 M. Ravasio , G. Tagliaferri , G. Ghisellini , F. Tavecchio , M. Boettcher , M. Sikora

The BL Lac 1ES 2344+514 is known for temporary extreme properties (e.g., a shift of the synchrotron SED peak energy $\nu_{synch,p}$ above 1keV). While those extreme states were so far observed only during high flux levels, additional…

High Energy Astrophysical Phenomena · Physics 2024-02-14 H. Abe , S. Abe , V. A. Acciari , I. Agudo , T. Aniello , S. Ansoldi , L. A. Antonelli , A. Arbet Engels , C. Arcaro , M. Artero , K. Asano , D. Baack , A. Babić , A. Baquero , U. Barres de Almeida , I. Batković , J. Baxter , J. Becerra González , E. Bernardini , J. Bernete , A. Berti , J. Besenrieder , C. Bigongiari , A. Biland , O. Blanch , G. Bonnoli , Ž Bošjak , I. Burelli , G. Busetto , A. Campoy-Ordaz , A. Carosi , R. Carosi , M. Carretero-Castrillo , A. J. Castro-Tirado , Y. Chai , A. Cifuentes , S. Cikota , E. Colombo , J. L. Contreras , J. Cortina , S. Covino , G. D'Amico , F. D'Ammando , V. D'Elia , P. Da Vela , F. Dazzi , A. De Angelis , B. De Lotto , A. Del Popolo , M. Delfino , J. Delgado , C. Delgado Mendez , D. Depaoli , F. Di Pierro , L. Di Venere , D. Dominis Prester , D. Dorner , M. Doro , D. Elsaesser , G. Emery , J. Escudero , L. Fariña , A. Fattorini , L. Foffano , L. Font , S. Fukami , Y. Fukazawa , R. J. García López , S. Gasparyan , M. Gaug , J. G. Giesbrecht Paiva , N. Giglietto , F. Giordano , P. Gliwny , R. Grau , J. G. Green , D. Hadasch , A. Hahn , L. Heckmann , J. Herrera , D. Hrupec , M. Hütten , R. Imazawa , T. Inada , R. Iotov , K. Ishio , I. Jiménez Martínez , J. Jormanainen , D. Kerszberg , G. W. Kluge , Y. Kobayashi , P. M. Kouch , H. Kubo , J. Kushida , M. Láinez Lezáun , A. Lamastra , F. Leone , E. Lindfors , L. Linhoff , S. Lombardi , F. Longo , M. López-Moya , A. López-Oramas , S. Loporchio , A. Lorini , B. Machado de Oliveira Fraga , P. Majumdar , M. Makariev , G. Maneva , N. Mang , M. Manganaro , M. Mariotti , M. Martínez , M. Martínez-Chicharro , A. Mas-Aguilar , D. Mazin , S. Menchiari , S. Mender , D. Miceli , T. Miener , J. M. Miranda , R. Mirzoyan , M. Molero González , E. Molina , H. A. Mondal , A. Moralejo , D. Morcuende , T. Nakamori , C. Nanci , V. Neustroev , C. Nigro , L. Nikolić , K. Nishijima , T. Njoh Ekoume , K. Noda , S. Nozaki , Y. Ohtani , A. Okumura , J. Otero-Santos , S. Paiano , M. Palatiello , D. Paneque , R. Paoletti , J. M. Paredes , D. Pavlović , M. Persic , M. Pihet , G. Pirola , F. Podobnik , P. G. Prada Moroni , E. Prandini , G. Principe , C. Priyadarshi , W. Rhode , M. Ribó , J. Rico , C. Righi , N. Sahakyan , T. Saito , K. Satalecka , F. G. Saturni , B. Schleicher , K. Schmidt , F. Schmuckermaier , J. L. Schubert , T. Schweizer , A. Sciaccaluga , J. Sitarek , A. Spolon , A. Stamerra , J. Strišović , D. Strom , Y. Suda , H. Tajima , R. Takeishi , F. Tavecchio , P. Temnikov , K. Terauchi , T. Terzić , M. Teshima , L. Tosti , S. Truzzi , A. Tutone , S. Ubach , J. van Scherpenberg , S. Ventura , V. Verguilov , I. Viale , C. F. Vigorito , V. Vitale , R. Walter , C. Wunderlich , T. Yamamoto M. Perri F. Verrecchia C. Leto , S. Das , R. Chatterjee , C. M. Raiteri , M. Villata , E. Semkov , S. Ibryamov , R. Bachev , A. Strigachev , G. Damljanovic , O. Vince , M. D. Jovanovic , M. Stojanovic , V. M. Larionov , T. S. Grishina , E. N. Kopatskaya , E. G. Larionova , D. A. Morozova , S. S. Savchenko , I. S. Troitskiy , Y. V. Troitskaya , A. A. Vasilyev , W. P. Chen , W. J. Hou , C. S. Lin , A. Tsai , S. G. Jorstad , Z. R. Weaver , J. A. Acosta-Pulido , M. I. Carnerero , D. Carosati , S. O. Kurtanidze , O. M. Kurtanidze , B. Jordan , R. Z. Ivanidze , K. Gazeas , K. Vrontaki , T. Hovatta , I. Liodakis , A. C. S. Readhead , S. Kiehlmann , W. Zheng , A. V. Filippenko

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