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Tadayuki Takahashi

4 papers hereh-index 111.6k citations28 works total

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

author position
  • middle author1

Across the 1 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
same name
  • Tadayuki Takahashi — 55 papers, h 71
  • Tadayuki Takahashi — 26 papers
  • Tadayuki Takahashi — 7 papers, h 22
  • Tadayuki Takahashi — 7 papers, h 4
  • Tadayuki Takahashi — 4 papers, h 9
  • Tadayuki Takahashi — 3 papers, h 8

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

most citedEvidence of 100 TeV γ-ray emission from HESS J1702-420: A new PeVatron candidate

24 citations · 45 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2023

Joint H.E.S.S. and Fermi-LAT analysis of the region around PSR J1813-1749

T. Wach, A. M. W. Mitchell, V. Joshi +1

HESS J1813-178 is one of the brightest sources detected during the first HESS Galactic Plane survey. The compact source, also detected by MAGIC, is believed to be a pulsar wind neb…

astro-ph.HE2023★ 19 cited

The Compton Spectrometer and Imager

John A. Tomsick, Steven E. Boggs, Andreas Zoglauer +72

The Compton Spectrometer and Imager (COSI) is a NASA Small Explorer (SMEX) satellite mission in development with a planned launch in 2027. COSI is a wide-field gamma-ray telescope…

astro-ph.HE2021★ 2 cited

The young massive stellar cluster Westerlund 1 in γ rays as seen with H.E.S.S

Lars Mohrmann, Andreas Specovius, Romed Rauth +2

Massive stellar clusters have recently been hypothesised as candidates for the acceleration of hadronic cosmic rays up to PeV energies. Previously, the H.E.S.S. Collaboration has r…

astro-ph.HE2021★ 24 cited

Evidence of 100 TeV γ-ray emission from HESS J1702-420: A new PeVatron candidate

H. Abdalla, F. Aharonian, F. Ait Benkhali +232

The identification of PeVatrons, hadronic particle accelerators reaching the knee of the cosmic ray spectrum (few 1015 eV), is crucial to understand the origin of cosmic rays…

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