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researcher

S. Vaughan

69 papers hereh-index 406.9k citations118 works total

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

author position
  • sole author2
  • first author7
  • middle author27
  • last author13

Across the 49 of 69 papers where every author was matched, so the position is known.

fields
  • astro-ph35
  • astro-ph.HE22
  • astro-ph.GA6
  • astro-ph.IM4
  • astro-ph.CO2
same name
  • S. Vaughan — 39 papers, h 11
  • S. Vaughan — 22 papers, h 12
  • S. Vaughan — 13 papers, h 5
  • S. Vaughan — 7 papers, h 4
  • S. Vaughan — 2 papers
  • S. Vaughan — 2 papers, h 3

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
19992020
most citedThe Ultraluminous State

463 citations · 6.1k across the 68 of their papers we have counts for

collaborators
Showing 2008Show all

4 papers · 1 filter

astro-ph2008★ 55 cited

A Comprehensive X-ray Spectral Analysis of the Seyfert 1.5 NGC 3227

A. Markowitz, J. N. Reeves, I. M. George +5

We present results of a 100 ks XMM observation of the Seyfert 1.5 NGC 3227. Our best-fit broadband model to the pn spectrum consists of a moderately flat (photon index 1.57) hard X…

astro-ph2008★ 50 cited

On the evidence for narrow, relativistically shifted X-ray lines

S. Vaughan, P. Uttley

In recent years there have been many reported detections of highly redshifted or blueshifted narrow spectral lines (both emission or absorption) in the X-ray spectra of active gala…

astro-ph2008★ 45 cited

Line Searches in Swift X-ray Spectra

C. P. Hurkett, S. Vaughan, J. P. Osborne +14

Prior to the launch of the Swift mission several X-ray line detections were reported in Gamma Ray Burst afterglow spectra. To date, these pre-Swift era results have not been conclu…

astro-ph2008★ 2 cited

Studying accreting black holes and neutron stars with time series: beyond the power spectrum

S. Vaughan, P. Uttley

The fluctuating brightness of cosmic X-ray sources, particularly accreting black holes and neutron star systems, has enabled enormous progress in understanding the physics of turbu…

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