Böck, M.Kadler, M.Müller, C.Tosti, G.Bastieri, D.Burnett, T.Carpenter, B.Cavazzuti, E.Dutka, M.Blanchard, J.Edwards, P. G.Hase, H.Horiuchi, S.Jauncey, D. L.Krauß, F.Lister, M. L.Lovell, J. E. J.Lott, B.Murphy, D. W.Phillips, C.Plötz, C.Pursimo, T.Quick, J.Ros, E.Taylor, G.Thompson, D. J.Tingay, S. J.Tzioumis, A.Zensus, J. A.2020-04-272020-04-272016-05-04M. Böck, M. Kadler, C. Müller, G. Tosti, R. Ojha, J. Wilms, D. Bastieri, T. Burnett, B. Carpenter, E. Cavazzuti, M. Dutka, J. Blanchard, P. G. Edwards, H. Hase, S. Horiuchi, D. L. Jauncey, F. Krauß, M. L. Lister, J. E. J. Lovell, B. Lott, D. W. Murphy, C. Phillips, C. Plötz, T. Pursimo, J. Quick, E. Ros, G. Taylor, D. J. Thompson, S. J. Tingay, A. Tzioumis and J. A. Zensus ,Radio and gamma-ray properties of extragalactic jets from the TANAMI sample, A&A, 590 (2016) A40 DOI: https://doi.org/10.1051/0004-6361/201424773https://doi.org/10.1051/0004-6361/201424773http://hdl.handle.net/11603/18288http://simbad.u-strasbg.fr/simbad/sim-ref?querymethod=bib&simbo=on&submit=submit+bibcode&bibcode=2016A%26A...590A..40Bhttps://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Search&refcode=2016A%26A...590A..40BThe TANAMI program has been observing parsec-scale radio jets of southern (declination south of − 30°) γ-ray bright AGN, simultaneously with Fermi/LAT monitoring of their γ-ray emission, via high-resolution radio imaging with Very Long Baseline Interferometry techniques. We present the radio and γ-rayproperties of the TANAMI sources based on one year of contemporaneous TANAMI and Fermi/LAT data. A large fraction (72%) of the TANAMI sample can be associated with bright γ-ray sources for this time range. Association rates differ for different optical classes with all BL Lacs, 76% of quasars, and just 17% of galaxies detected by the LAT. Upper limits were established on the γ-ray flux from TANAMI sources not detected by LAT. This analysis led to the identification of three new Fermi sources whose detection was later confirmed. The γ-ray and radio luminosities are related by Lγ ∝ Lᵣ⁰·⁸⁹±⁰·⁰⁴. The brightness temperatures of the radio cores increase with the average γ-ray luminosity and the presence of brightness temperatures above the inverse Compton limit implies strong Doppler boosting in those sources. The undetected sources have lower γ/radio luminosity ratios and lower contemporaneous brightness temperatures. Unless the Fermi/LAT-undetected blazars are much γ-ray-fainter than the Fermi/LAT-detected sources, their γ-ray luminosity should not be significantly lower than the upper limits calculated here.12 pagesen-USThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.© ESO 2016Text