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researcher

Y. Uchiyama

18 papers hereh-index 232.9k citations37 works total

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

author position
  • middle author3
  • last author2

Across the 5 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE12
  • astro-ph2
  • astro-ph.GA2
  • astro-ph.EP1
  • astro-ph.IM1
same name
  • Y. Uchiyama — 193 papers, h 88
  • Y. Uchiyama — 54 papers, h 19
  • Y. Uchiyama — 29 papers, h 22
  • Y. Uchiyama — 6 papers
  • Y. Uchiyama — 6 papers, h 22
  • Y. Uchiyama — 5 papers

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
20062017
most citedHard X-ray Detector (HXD) on Board Suzaku

647 citations · 1.6k across the 18 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.HE2014

ASTRO-H White Paper - Shock and Acceleration

F. Aharonian, Y. Uchiyama, D. Khangulyan +4

We discuss the prospects for a progress to be brought by ASTRO-H in the understanding of the physics of particle acceleration in astrophysical environments. Particular emphasis wil…

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…

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