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researcher

Mark R. Swain

4 papers hereh-index 9435 citations14 works total

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

author position
  • first author1
  • middle author2
  • last author1

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

fields
  • astro-ph4
same name
  • Mark R. Swain — 1 paper, h 2

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
20032008
most citedChandra Reveals Twin X-ray Jets in the Powerful FR-II Radio Galaxy 3C353

45 citations · 52 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph2008★ 45 cited

Chandra Reveals Twin X-ray Jets in the Powerful FR-II Radio Galaxy 3C353

J. Kataoka, L. Stawarz, D. E. Harris +7

We report X-ray imaging of the powerful FR-II radio galaxy 3C353 using the Chandra X-ray Observatory. 3C353's two 4"-wide and 2'-long jets allow us to study in detail the internal…

astro-ph2007★ 7 cited

Nulling interferometry: performance comparison between Antarctica and other ground-based sites

O. Absil, V. Coude du Foresto, M. Barillot +1

Detecting the presence of circumstellar dust around nearby solar-type main sequence stars is an important pre-requisite for the design of future life-finding space missions such as…

astro-ph2005

Keck Interferometer Observations of FU Orionis Objects

R. Millan-Gabet, J. D. Monnier, R. L. Akeson +31

We present new K-band long baseline interferometer observations of three young stellar objects of the FU Orionis class, V1057 Cyg, V1515 Cyg and Z CMa-SE, obtained at the Keck Inte…

astro-ph2003

Interferometer Observations of Subparsec-scale Infrared Emission in the Nucleus of NGC 4151

M. Swain, G. Vasisht, R. Akeson +22

We report novel, high-angular resolution interferometric measurements that imply the near-infrared nuclear emission in NGC 4151 is unexpectedly compact. We have observed the nucleu…

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