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researcher

S. O'Sullivan

14 papers hereh-index 7350 citations10 works total

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

author position
  • first author3
  • middle author8
  • last author1

Across the 12 of 14 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO4
  • astro-ph.HE3
  • astro-ph.IM3
  • astro-ph.EP2
  • astro-ph.GA2
same name
  • S. O'Sullivan — 14 papers, h 12
  • S. O'Sullivan — 11 papers, h 1
  • S. O'Sullivan — 6 papers, h 4
  • S. O'Sullivan — 1 paper, h 2
  • S. O'Sullivan — 1 paper, h 0

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20112026
most citedComplex Faraday depth structure of Active Galactic Nuclei as revealed by broadband radio polarimetry

181 citations · 876 across the 14 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2018★ 12 cited

Faraday rotation study of NGC 612 (PKS 0131-36): a hybrid radio source and its magnetised circumgalactic environment

J. K. Banfield, S. P. O'Sullivan, M. H. Wieringa +1

We present a polarization and Faraday rotation study of the hybrid morphology radio galaxy NGC 612 (PKS 0131-36), using Australian Telescope Compact Array observations from 1 to 3…

astro-ph.HE2018★ 31 cited

Broadband radio polarimetry of Fornax A, I: Depolarized patches generated by advected thermal material from NGC 1316

C. S. Anderson, B. M. Gaensler, G. H. Heald +3

We present observations and analysis of the polarized radio emission from the nearby radio galaxy Fornax A over 1.28--3.1 GHz, using data from the Australia Telescope Compact Array…

astro-ph.HE2013★ 29 cited

Broadband radio circular polarization spectrum of the relativistic jet in PKS B2126-158

S. P. O'Sullivan, N. M. McClure-Griffiths, I. J. Feain +2

We present full-Stokes radio polarization observations of the quasar PKS B2126-158 (z=3.268) from 1 to 10 GHz using the Australia Telescope Compact Array. The source has large frac…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.