Simultaneous Radio to (Sub-) mm-Monitoring of Variability and Spectral Shape Evolution of potential GLAST Blazars

Abstract

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 7 mm 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’ radio bands. Further we will give a brief outlook including the extension of this coordinated campaign towards higher frequencies and future scientific aims.