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Radio and Gamma-ray Properties of Extragalactic Jets from the TANAMI Sample
- Source :
- A&A 590, A40 (2016)
- Publication Year :
- 2016
-
Abstract
- Using high-resolution radio imaging with VLBI techniques, the TANAMI program has been observing the parsec-scale radio jets of southern (declination south of -30{\deg}) gamma-ray bright AGN simultaneously with Fermi/LAT monitoring of their gamma-ray emission. We present the radio and gamma-ray properties 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 gamma-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 gamma-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 gamma-ray and radio luminosities are related by $L_\gamma \propto L_r^{0.89+-0.04}$. The brightness temperatures of the radio cores increase with the average gamma-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 gamma/radio luminosity ratios and lower contemporaneous brightness temperatures. Unless the Fermi/LAT-undetected blazars are strongly gamma-ray-fainter than the Fermi/LAT-detected ones, their gamma-ray luminosity should not be significantly lower than the upper limits calculated here.<br />Comment: 12 pages, 11 figures, 3 tables, Accepted for publication in Astronomy & Astrophysics
Details
- Database :
- arXiv
- Journal :
- A&A 590, A40 (2016)
- Publication Type :
- Report
- Accession number :
- edsarx.1601.05099
- Document Type :
- Working Paper
- Full Text :
- https://doi.org/10.1051/0004-6361/201424773