The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future blazar studies. In order to fully benefit from its capabilities and to maximize the scientific return from the LAT, it is of great importance to conduct dedicated multi-frequency monitoring campaigns that will result comprehensive observations. Consequently, we initiated an effort to conduct a GLAST-dedicated, quasi-simultaneous, broad-band flux-density (and polarization) monitoring of potential GLAST blazars with the Effelsberg and OVRO radio telescopes (11 cm to 7mm wavelength). Here, we present a short overview of these activities which will complement the multi-wavelengths activities of the GLAST/LAT collaboration towards the 'low-energy' ...
known blazars, yet the existing experimental set of data does not allow one to make unambiguous stat...
Aims. A huge multiwavelength campaign targeting the blazar AO 0235+164 was organized by the Whole Ea...
Context. After years of modest optical activity, the quasar-type blazar 4C 38.41 (B3 1633+382) exper...
The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future b...
Aims. Since the CGRO operation in 1991–2000, one of the primary unresolved questions about the blaza...
We are monitoring 29 blazars with monthly VLBA polarimetric imaging at 43 GHz, occasional VLBA imagi...
One of the more notable features of the Large Area Telescope (LAT) on GLAST is its extremely large f...
The Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope provides an unprecedented ...
The OVRO 40 m Telescope monitoring program carries out twice-weekly measurements of the 15 GHz flux ...
We present an analysis of the multiwavelength behaviour of the blazar OJ 248 at z = 0.939 in the per...
Systematic monitoring of specific targets in the optical regime was historically applied on a very n...
Since late 2007, we have been monitoring a large sample of known and likely gamma-ray–loud blazars a...
© 2015 The Authors. We present an analysis of the multiwavelength behaviour of the blazar OJ 248 at ...
Variability is an important and defining characteristic of AGN, that along with their broadband spec...
Context: Being dominated by non-thermal emission from aligned relativistic jets, blazars allow us to...
known blazars, yet the existing experimental set of data does not allow one to make unambiguous stat...
Aims. A huge multiwavelength campaign targeting the blazar AO 0235+164 was organized by the Whole Ea...
Context. After years of modest optical activity, the quasar-type blazar 4C 38.41 (B3 1633+382) exper...
The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future b...
Aims. Since the CGRO operation in 1991–2000, one of the primary unresolved questions about the blaza...
We are monitoring 29 blazars with monthly VLBA polarimetric imaging at 43 GHz, occasional VLBA imagi...
One of the more notable features of the Large Area Telescope (LAT) on GLAST is its extremely large f...
The Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope provides an unprecedented ...
The OVRO 40 m Telescope monitoring program carries out twice-weekly measurements of the 15 GHz flux ...
We present an analysis of the multiwavelength behaviour of the blazar OJ 248 at z = 0.939 in the per...
Systematic monitoring of specific targets in the optical regime was historically applied on a very n...
Since late 2007, we have been monitoring a large sample of known and likely gamma-ray–loud blazars a...
© 2015 The Authors. We present an analysis of the multiwavelength behaviour of the blazar OJ 248 at ...
Variability is an important and defining characteristic of AGN, that along with their broadband spec...
Context: Being dominated by non-thermal emission from aligned relativistic jets, blazars allow us to...
known blazars, yet the existing experimental set of data does not allow one to make unambiguous stat...
Aims. A huge multiwavelength campaign targeting the blazar AO 0235+164 was organized by the Whole Ea...
Context. After years of modest optical activity, the quasar-type blazar 4C 38.41 (B3 1633+382) exper...