Context. BL Lacertae objects are variable at all energy bands on time scales down to minutes. To construct and interpret their spectral energy distribution (SED), simultaneous broad-band observations are mandatory. Up to now, the number of objects studied during such campaigns is very limited and biased towards high flux states. Aims. We present the results of a dedicated multi-wavelength study of the high-frequency peaked BL Lacertae (HBL) object and known TeV emitter 1ES 2344+514 by means of a pre-organised campaign. Methods. The observations were conducted during simultaneous visibility windows of MAGIC and AGILE in late 2008. The measurements were complemented by Mets hovi, RATAN-600, KVA+Tuorla, Swift and VLBA pointings. Additional cov...
We report on the VERITAS observations of the high-frequency peaked BL Lac object 1ES 1959+650 in the...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in very high energy (...
Abstract: We present results of multi-wavelength (MWL) observations of the high-frequency-peaked BL ...
Context. BL Lacertae objects are variable at all energy bands on time scales down to minutes. To con...
Context. BL Lacertae objects are variable at all energy bands on time scales down to minutes. To con...
Context. BL Lacertae objects are variable at all energy bands on time scales down to minutes. To con...
Context. BL Lacertae objects are variable at all energy bands on time scales down to minut...
Context was to construct and interpret the spectral energy distribution (SED) of BL Lacertae objects...
Extreme High-frequency BL~Lacs (EHBL) feature their synchrotron peak of the broadband spectral energ...
[Abridged] Context. To construct and interpret the spectral energy distribution (SED) of BL Lacertae...
Extreme High-frequency BL Lacs (EHBL) feature their synchrotron peak of the broadband spectral energ...
The spectral energy distribution (SED) of high-frequency peaked BL Lac objects (HBL) is characterize...
Multiwavelength observations of the high-frequency-peaked blazar 1ES 2344+514 were performed from 20...
We report on the VERITAS observations of the high-frequency peaked BL Lac object 1ES 1959+650 in the...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in very high energy (...
Abstract: We present results of multi-wavelength (MWL) observations of the high-frequency-peaked BL ...
Context. BL Lacertae objects are variable at all energy bands on time scales down to minutes. To con...
Context. BL Lacertae objects are variable at all energy bands on time scales down to minutes. To con...
Context. BL Lacertae objects are variable at all energy bands on time scales down to minutes. To con...
Context. BL Lacertae objects are variable at all energy bands on time scales down to minut...
Context was to construct and interpret the spectral energy distribution (SED) of BL Lacertae objects...
Extreme High-frequency BL~Lacs (EHBL) feature their synchrotron peak of the broadband spectral energ...
[Abridged] Context. To construct and interpret the spectral energy distribution (SED) of BL Lacertae...
Extreme High-frequency BL Lacs (EHBL) feature their synchrotron peak of the broadband spectral energ...
The spectral energy distribution (SED) of high-frequency peaked BL Lac objects (HBL) is characterize...
Multiwavelength observations of the high-frequency-peaked blazar 1ES 2344+514 were performed from 20...
We report on the VERITAS observations of the high-frequency peaked BL Lac object 1ES 1959+650 in the...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in very high energy (...
Abstract: We present results of multi-wavelength (MWL) observations of the high-frequency-peaked BL ...