Radio and gamma-ray properties of extragalactic jets from the TANAMI sample

Böck, M.; Kadler, M.; Müller, C.; Tosti, G.; Ojha, R.; Wilms, J.; 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.

doi:10.1051/0004-6361/201424773

Title: Radio and gamma-ray properties of extragalactic jets from the TANAMI sample

Journal Article · Wed May 04 00:00:00 EDT 2016 · Astronomy and Astrophysics

DOI:https://doi.org/10.1051/0004-6361/201424773· OSTI ID:1355699

Böck, M.; Kadler, M.; Müller, C.; Tosti, G.; Ojha, R.; Wilms, J.; 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. more »

The 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. In this paper, 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 L_γ ∝ L_r^0.89±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. Finally, 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.

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Research Organization:: NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)

Sponsoring Organization:: USDOE; National Aeronautics and Space Administration (NASA); Federal Ministry for Economic Affairs and Energy (BMWi) (Germany); Ministry of Economy, Industry and Competitiveness (MINECO) (Spain); Generalitat Valenciana; European Cooperation in Science and Technology (COST) (Belgium)

Contributing Organization:: Fermi LAT Collaboration

Grant/Contract Number:: AC02-76SF00515; NNH09ZDA001N; NNH10ZDA001N; 50OR0808; AYA2009-13036-C02-C02; AYA2012-38491-C02-01; Prometeo 2009/104; MP0905

OSTI ID:: 1355699

Journal Information:: Astronomy and Astrophysics, Vol. 590; ISSN 0004-6361

Publisher:: EDP SciencesCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 11 works

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Mid-infared Light Curve and High-resolution Radio Structure of the Candidate Neutrino Source GB6 J1040+0617 Gabányi, Krisztina É.; Frey, Sándor; Moór, Attila Research Notes of the AAS, Vol. 3, Issue 2 https://doi.org/10.3847/2515-5172/ab074d	journal	February 2019
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79 ASTRONOMY AND ASTROPHYSICS
galaxies: active
galaxies: nuclei
galaxies: jets
gamma rays: galaxies
radio continuum: galaxies

Title: Radio and gamma-ray properties of extragalactic jets from the TANAMI sample

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