activity
20072009
most citedThree dimensional magnetic field structure of six parsec-scale active galactic nuclei jets

107 citations · 111 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2009

Simulation of the Polarized Sky at 1.4 GHz

S. P. O'Sullivan, J. M. Stil, A. R. Taylor +3

We present results from simulations of the extragalactic polarized sky at 1.4 GHz. As the basis for our polarization models, we use a semi-empirical simulation of the extragalactic…

astro-ph20082 cited

AGN jet physics from measurements of the frequency-dependent position of the VLBI radio core

Shane P. O'Sullivan, Denise C. Gabuzda

Accurate measurement of the frequency-dependent shift of the self-absorbed radio core is required for multi-frequency analysis of VLBI data since absolute positional information is…

astro-ph2008107 cited

Three dimensional magnetic field structure of six parsec-scale active galactic nuclei jets

Shane P. O'Sullivan, Denise C. Gabuzda

The parsec-scale Faraday rotation measure (RM) distribution of six "blazars" is investigated using multi-frequency (4.6--43 GHz) polarization observations taken on 2006 July 2 with…

astro-ph2008

The Need For High Resolution In Studies Of The 3-D Magnetic Field Structure Of AGN Jets

Shane P. O'Sullivan, Denise C. Gabuzda

We are using "broadband" (4.6 to 43 GHz) multi-frequency VLBA polarization observations of compact AGN to investigate the 3-D structure of their jet magnetic (B) fields. Observing…

astro-ph20082 cited

Parsec-scale Investigation of the Magnetic Field Structure of Several AGN Jets

Shane P. O'Sullivan, Denise C. Gabuzda

Multi-frequency (4.6, 5, 5.5, 8, 8.8, 13, 15, 22 & 43 GHz) polarization observations of 6 "blazars" were obtained on the American Very Long Baseline Array (VLBA) over a 24-hr perio…

astro-ph2007

Investigation of the Faraday Rotation Measure and Magnetic Field Structures of Several AGN Jets on Sub-Parsec to Parsec Scales

Shane P. O'Sullivan, Denise C. Gabuzda

Preliminary VLBA polarisation results on 6 ``blazars'' from 6.5-cm to 7-mm are presented here. Observing at several different wavelengths, separated by short and long intervals, en…