ATCA monitoring of gamma-ray loud AGN in support of the Fermi mission

Details ATCA monitoring of gamma-ray loud AGN in support of the Fermi mission ATCA monitoring of gamma-ray loud AGN in support of the Fermi mission

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atnf.prop.1995t&link_type=abstract

ATNF proposal C1730, Semester: April, 2009

Physics

Extragalactic, Atca

Scientific paper

Following a successful pilot investigation to determine the feasibility of monitoring bright gamma-ray AGN at 7 mm throughout the year (C1730), we propose a continuation of the project into a one year phase of observations that will support the Fermi mission following its June 2008 launch. The goal of this project is to monitor Fermi-identified AGN at 4.8, 8.6, 17, 19, 38, and 40 GHz at monthly intervals, tracking variability in the AGN (in particular flaring activity) that can be related to gamma-ray variability observed by Fermi and pc-scale structural variability observed by our concurrent Southern Hemipshere VLBI monitoring program in support of Fermi. The ATCA, VLBI, and Fermi data will contribute to a multi-wavelength AGN database that will help us understand the origins of high energy emission in AGN.

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