VLBA22A-453

Tracking A Blazar Jet Ejection at Redshift 4.3

Abstract

We have detected a gamma-ray flare in the high-redshift blazar GB 1508+5714 (ATel #15202). At a redshift of z=4.3, the blazar is one of the most distant sources in the Universe that has been detected at gamma-ray energies and its recent gamma-ray flare provides a rare opportunity to study its broadband emission with simultaneous multi-wavelength data. We propose a multi-frequency VLBI follow-up campaign with the VLBA and the Effelsberg 100-m radio telescope at 15, 22, and 43 GHz and the additional participation of GBT at 86 GHz to detect possible newly-emerging components and to measure spectral variations of the most compact parts of the structure of the source. The object has at present a flat radio spectrum with about 200 mJy flux density (increasing). The proposed ToO VLBI observations will probe the ejection of plasma components in an AGN jet at a high rest-frame frequency of over 200 GHz (450 GHz with 86 GHz observations). At the lower observing frequencies, we will be able to compare the radio-to-gamma-ray properties of the jet ejections in today's blazars with those found in the early Universe.

Investigators

Name Institution
GBT Operator Green Bank Observatory
Florian Eppel Würzburg, Universität
Petra Benke Max-Planck-Institut für Radioastronomie
Joern Wilms Astronomical Institute of the University of Erlangen-Nuremburg
Florian Roesch Würzburg, Universität
Michael Kreter Würzburg, Universität
Jonas Hessdoerfer Würzburg, Universität
Jeffrey Hodgson Max-Planck-Institut für Radioastronomie; Korea Astronomy and Space Science Institute
Leonid Gurvits Joint Institute for Very Long Baseline Interferometry European Research Infrastructure Consortium
Yuri Kovalev Max-Planck-Institut für Radioastronomie
Eduardo Ros Max-Planck-Institut für Radioastronomie; València, Universitat de
Mikhail Lisakov Max-Planck-Institut für Radioastronomie; Lebedev Physical Institute
Andrea Gokus * Washington University in St. Louis
Matthias Kadler Würzburg, Universität

* indicates the PI