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A. Sutton

18 papers hereh-index 14886 citations29 works total

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

author position
  • first author7
  • middle author7
  • last author3

Across the 17 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE16
  • astro-ph.CO1
  • astro-ph.GA1
same name
  • A. Sutton — 21 papers, h 11
  • A. Sutton — 4 papers, h 47
  • A. Sutton — 4 papers, h 14
  • A. Sutton — 4 papers
  • A. Sutton — 2 papers, h 97
  • A. Sutton — 2 papers, 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
20102016
most citedThe ultraluminous state revisited: fractional variability and spectral shape as diagnostics of super-Eddington accretion

255 citations · 1.2k across the 17 of their papers we have counts for

collaborators
Showing 2013 · astro-ph.HEShow all

3 papers · 2 filters

astro-ph.HE2013★ 55 cited

Radio observations of extreme ULXs: revealing the most powerful ULX radio nebula ever or the jet of an intermediate-mass black hole?

M. Mezcua, T. P. Roberts, A. D. Sutton +1

The most extreme ultraluminous X-ray sources (ULXs), with LX​>5×1040 erg s−1, are amongst the best candidates for hosting intermediate-mass black holes…

astro-ph.HE2013★ 255 cited

The ultraluminous state revisited: fractional variability and spectral shape as diagnostics of super-Eddington accretion

Andrew D. Sutton, Timothy P. Roberts, Matthew J. Middleton

Although we are nearing a consensus that most ULXs are stellar-mass black holes in a super-Eddington state, little is yet established of the physics of this accretion mode. Here, w…

astro-ph.HE2013★ 37 cited

A bright ultraluminous X-ray source in NGC 5907

Andrew D. Sutton, Timothy P. Roberts, Jeanette C. Gladstone +4

We present a multi-mission X-ray analysis of a bright (peak observed 0.3-10 keV luminosity of ~ 6x10^{40} erg s^{-1}), but relatively highly absorbed ULX in the edge-on spiral gala…

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