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Y. Komori

6 papers hereh-index 11800 citations68 works total

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

author position
  • first author1
  • middle author5

Across the 6 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.HE2
  • hep-ex1
same name
  • Y. Komori — 136 papers
  • Y. Komori — 26 papers, h 16
  • Y. Komori — 6 papers, h 15
  • Y. Komori — 6 papers
  • Y. Komori — 5 papers, h 9
  • Y. Komori — 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
20022012
most citedThe Most Likely Sources of High Energy Cosmic-Ray Electrons in Supernova Remnants

227 citations · 373 across the 6 of their papers we have counts for

collaborators
Showing astro-phShow all

3 papers · 1 filter

astro-ph2008★ 108 cited

High-energy electron observations by PPB-BETS flight in Antarctica

S. Torii, T. Yamagami, T. Tamura +23

We have observed cosmic-ray electrons from 10 GeV to 800 GeV by a long duration balloon flight using Polar Patrol Balloon (PPB) in Antarctica. The observation was carried out for 1…

astro-ph2006★ 9 cited

Cosmic-ray spectra of primary protons and high altitude muons deconvolved from observed atmospheric gamma rays

K. Yoshida, R. Ohmori, T. Kobayashi +3

We have observed atmospheric gamma rays from 30GeV to 8TeV, using emulsion chambers at balloon altitudes, accumulating the largest total exposure in this energy range to date, SOT…

astro-ph2003★ 227 cited

The Most Likely Sources of High Energy Cosmic-Ray Electrons in Supernova Remnants

T. Kobayashi, Y. Komori, K. Yoshida +1

Evidences of non-thermal X-ray emission and TeV gamma-rays from the supernova remnants (SNRs) has strengthened the hypothesis that primary Galactic cosmic-ray electrons are acceler…

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