GMVA14B-428

3 mm Imaging of the Most Compact Regions of Gamma-Ray Blazars

Abstract

We propose to image 16 gamma-ray bright blazars at 3 mm during the GMVA sessions in autumn 2014 & spring 2015. A major goal is to refine the data processing and imaging procedures for short mm-wave VLBI to help the development of 1 mm VLBI. The same objects are monitored monthly with the VLBA at 7 mm to follow the time evolution of the jet and continuously at gamma-ray energies with Fermi as well as at intermediate wavebands with a wide variety of instruments. Another aim of the GMVA observations is to identify how the high-energy emission relates to moving & stationary shock waves, bends, and other physical structures in the core region. We will accomplish this by total and polarized intensity imaging with angular resolution of about 50 microarcsec. The 3 mm images will (1) probe the core region where opacity and limited resolution make this difficult at 7 mm, (2) provide angular sizes and spectra of the most compact features for determining physical parameters, and (3) measure the polarization of core and inner jet at 86 GHz, which can be compared with those at 43 GHz (VLBA) and at 22 GHz (RadioAstron + ground arrays).

Investigators

Name Institution
Michael Bremer Institut de Radio Astronomique Millimétrique
Yuri Kovalev Max-Planck-Institut für Radioastronomie
Andrei Lobanov Max-Planck-Institut für Radioastronomie
Nicholas MacDonald Boston University; Max-Planck-Institut für Radioastronomie; Mississippi, University of
Mason Keck Boston University
Ivan Agudo Boston University; Joint Institute for Very Long Baseline Interferometry European Research Infrastructure Consortium; Andalucía, Instituto de Astrofísica de; Andalucía, Instituto de Astrofísica de
Bindu Rani Max-Planck-Institut für Radioastronomie
Jose L. Gomez Andalucía, Instituto de Astrofísica de
Svetlana Jorstad Boston University
Jeffrey Hodgson Max-Planck-Institut für Radioastronomie; Korea Astronomy and Space Science Institute
Thomas Krichbaum Max-Planck-Institut für Radioastronomie
Alan Marscher * Boston University
GBT Operator Green Bank Observatory

* indicates the PI