Extragalactic Jets from the TANAMI Sample as Seen by Fermi/LAT
Moritz Boeck, Matthias Kadler, Gino Tosti, Toby Burnett, Roopesh Ojha,, Cornelia Mueller, Joern Wilms

TL;DR
This paper analyzes gamma-ray emissions from southern AGN jets monitored by TANAMI and Fermi/LAT, providing insights into their gamma-ray properties and upper flux limits for non-detected sources.
Contribution
It offers the first comprehensive gamma-ray analysis of TANAMI southern AGN jets using Fermi/LAT data, including flux upper limits for undetected sources.
Findings
Identification of gamma-ray bright AGN in the TANAMI sample
Upper limits on gamma-ray flux for non-detected sources
Characterization of gamma-ray properties of southern AGN jets
Abstract
The TANAMI program has been monitoring the parsec-scale radio jets of southern gamma-ray bright AGN with VLBI techniques simultaneously with Fermi/LAT monitoring of their gamma-ray emission. Here we present the gamma-ray properties of the TANAMI sources based on an analysis of the preliminary 1-year LAT source list. We present upper limits on the gamma-ray flux for TANAMI sources not detected by LAT.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Gamma-ray bursts and supernovae
