We performed an observational program with the X-ray satellite BeppoSAX, to study objects with extreme synchrotron peak frequencies ($\nu_{\rm peak}> 1$ keV). Of the seven sources observed, five revealed or confirmed their extreme nature. Four showed peak frequencies in the range 1-5 keV, while one (1ES 1426+428) displayed a flat power law spectrum ($\alpha_{\rm x}=0.92\pm0.04$) which locates its synchrotron peak at or above 100 keV. This is the third source of this type ever found, after Mkn 501 and 1ES 2344+514. In the context of the whole blazar class, the broad band properties of these objects confirm the scenario of a synchrotron peak smoothly spanning the IR -X-ray range, which explains the multi-frequency properties of the ...
We present recent ROSAT, ASCA and SAX observations of intermediate BL Lac objects (IBLs), i.e. BL La...
The BL Lac object 1ES 1011+496 was discovered at very high energy (VHE, E > 100GeV) γ-rays by Major ...
The bright BL Lac object PKS 2005-489 was observed by BeppoSAX on November 1-2, 1998, following an a...
We performed an observational program with the X-ray satellite BeppoSAX, to study objects with extr...
We performed an observational program with the X-ray satellite BeppoSAX, to study objects with extre...
The blazar 1ES 0229+200 is a high-frequency-peaked BL Lac object with a hard TeV spectrum extending ...
The multi-frequency “Sedentary Survey” is a deep, statistically complete, radio flux limited sample...
Extreme high-frequency BL Lacs (EHBL) feature their synchrotron peak of the broad-band spectral ener...
The BL Lac object 1ES 1011+496 was discovered at very high energy (VHE, E > 100GeV) \u3b3-rays by Ma...
The multi-frequency `Sedentary Survey' is a deep, statistically complete, radio flux limited sample ...
Extreme High-frequency BL Lacs (EHBL) feature their synchrotron peak of the broadband spectral energ...
The blazar 1ES 1959+650 was observed twice by BeppoSAX in September 2001 simultaneously with optical...
Context. Blazars are the dominant type of extragalactic sources at microwave and at γ-ray energies. ...
All but three (M87, BL Lac, and 3C 279) extragalactic sources detected so far at very high energy ga...
Extreme high-frequency-peaked BL Lac objects (EHBLs) are the most energetic persistent sources in th...
We present recent ROSAT, ASCA and SAX observations of intermediate BL Lac objects (IBLs), i.e. BL La...
The BL Lac object 1ES 1011+496 was discovered at very high energy (VHE, E > 100GeV) γ-rays by Major ...
The bright BL Lac object PKS 2005-489 was observed by BeppoSAX on November 1-2, 1998, following an a...
We performed an observational program with the X-ray satellite BeppoSAX, to study objects with extr...
We performed an observational program with the X-ray satellite BeppoSAX, to study objects with extre...
The blazar 1ES 0229+200 is a high-frequency-peaked BL Lac object with a hard TeV spectrum extending ...
The multi-frequency “Sedentary Survey” is a deep, statistically complete, radio flux limited sample...
Extreme high-frequency BL Lacs (EHBL) feature their synchrotron peak of the broad-band spectral ener...
The BL Lac object 1ES 1011+496 was discovered at very high energy (VHE, E > 100GeV) \u3b3-rays by Ma...
The multi-frequency `Sedentary Survey' is a deep, statistically complete, radio flux limited sample ...
Extreme High-frequency BL Lacs (EHBL) feature their synchrotron peak of the broadband spectral energ...
The blazar 1ES 1959+650 was observed twice by BeppoSAX in September 2001 simultaneously with optical...
Context. Blazars are the dominant type of extragalactic sources at microwave and at γ-ray energies. ...
All but three (M87, BL Lac, and 3C 279) extragalactic sources detected so far at very high energy ga...
Extreme high-frequency-peaked BL Lac objects (EHBLs) are the most energetic persistent sources in th...
We present recent ROSAT, ASCA and SAX observations of intermediate BL Lac objects (IBLs), i.e. BL La...
The BL Lac object 1ES 1011+496 was discovered at very high energy (VHE, E > 100GeV) γ-rays by Major ...
The bright BL Lac object PKS 2005-489 was observed by BeppoSAX on November 1-2, 1998, following an a...