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The gamma-ray properties of radio-selected extragalactic jets

Most extragalactic jets in radio-loud Active Galactic Nuclei are bright and variable gamma-ray sources, which are continuously monitored with Fermi/LAT. We present the gamma-ray properties of the MOJAVE and TANAMI AGN samples of radio-loud AGN. Both programs provide properties of the parsec-scale radio jets using Very Long Baseline Interferometry (VLBI) techniques. This information is important to understand the broad-band emission mechanism of these sources. In this work we compare the radio and gamma -ray properties of the two samples and present upper limits on the gamma-ray flux of the radio-brightest jet sources not yet detected by Fermi/LAT.

preprint2010arXivOpen access
M. BoeckM. KadlerG. TostiT. H. BurnettC. MuellerR. OjhaJ. Wilms
astro-ph.COastro-ph.HE
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M. BoeckM. KadlerG. TostiT. H. BurnettC. MuellerR. OjhaJ. Wilms

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