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S. P. O’Sullivan

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author3
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.CO1
ORCID 0000-0002-3968-3051

identity via Semantic Scholar / OpenAlex

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

107 citations · 130 across the 4 of their papers we have counts for

collaborators

4 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-ph2008★ 2 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-ph2008★ 107 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★ 21 cited

Environmental limits on the non-resonant cosmic-ray current-driven instability

B. Reville, J. G. Kirk, P. Duffy +1

We investigate the so-called non-resonant cosmic-ray streaming instability, first discussed by Bell (2004). The extent to which thermal damping and ion-neutral collisions reduce th…

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