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Radio-optical-gamma-ray properties of MOJAVE AGN detected byFermi/LAT

2011/04/30 by T. G. Arshakian, J. León-Tavares, M. Boettcher +7 · 1 citation
Physics and Astronomy · #Accretion (finance) #Active galactic nucleus #Astronomy #Astrophysical jet #Astrophysics #Astrophysics and Cosmic Phenomena #Blazar #Dark Matter and Cosmic Phenomena #Fermi Gamma-ray Space Telescope #Galaxy #Gamma ray #Jet (fluid) #Lorentz factor #Lorentz transformation #Luminosity #Physics #Quasar #Radio Astronomy Observations and Technology #Radio galaxy #Superluminal motion #astro-ph.CO

paper · pdf · doi:10.1051/0004-6361/201117140

13 pages, 10 figures, 4 tables, after moderate revision the paper is accepted for publication in A&A

arxiv created 2011/10/24 · openalex publication_date 2011/10/24 · arxiv updated 2015/05/28 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We use a sample of 83 core-dominated active galactic nuclei (AGN) selected from the MOJAVE (Monitoring of Jets in AGN with VLBA Experiments) radio-flux-limited sample and detected with the Fermi Large Area Telescope (LAT) to study the relations between non-simultaneous radio, optical, and γ-ray measurements.

Citations

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