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John P. Hughes

16 papers hereh-index 11730 citations21 works total

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

author position
  • middle author4
  • last author1

Across the 5 of 16 papers where every author was matched, so the position is known.

fields
  • astro-ph9
  • astro-ph.HE5
  • astro-ph.CO1
  • astro-ph.IM1
same name
  • John P. Hughes — 11 papers, h 5
  • John P. Hughes — 10 papers
  • John P. Hughes — 2 papers, h 3
  • John P. Hughes — 1 paper, h 1
  • John P. Hughes — 1 paper, 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
20012014
most citedA High-Resolution Study of Nonthermal Radio and X-Ray Emission from SNR G347.3-0.5

134 citations · 801 across the 16 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.HE2014★ 3 cited

ASTRO-H White Paper - Young Supernova Remnants

J. P. Hughes, S. Safi-Harb, A. Bamba +23

Thanks to the unprecedented spectral resolution and sensitivity of the Soft X-ray Spectrometer (SXS) to soft thermal X-ray emission, ASTRO-H will open a new discovery window for un…

astro-ph.HE2014★ 1 cited

ASTRO-H White Paper - Older Supernova Remnants and Pulsar Wind Nebulae

K. S. Long, A. Bamba, F. Aharonian +20

Most supernova remnants (SNRs) are old, in the sense that their structure has been profoundly modified by their interaction with the surrounding interstellar medium (ISM). Old SNRs…

astro-ph.HE2014★ 6 cited

A CR-hydro-NEI Model of the Structure and Broadband Emission from Tycho's SNR

P. Slane, S. -H. Lee, D. C. Ellison +5

Tycho's supernova remnant (SNR) is well-established as a source of particle acceleration to very high energies. Constraints from numerous studies indicate that the observed gamma-r…

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