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researcher

T. Takahashi

34 papers hereh-index 00 citations0 works total

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

author position
  • middle author9
  • last author4

Across the 13 of 34 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE20
  • astro-ph8
  • astro-ph.CO4
  • astro-ph.GA1
  • astro-ph.IM1
same name
  • T. Takahashi — 71 papers, h 20
  • T. Takahashi — 42 papers, h 42
  • T. Takahashi — 41 papers, h 41
  • T. Takahashi — 36 papers
  • T. Takahashi — 19 papers, h 9
  • T. Takahashi — 12 papers, h 34

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
19962021
most citedA short gamma-ray burst apparently asssociated with an elliptical galaxy at redshift z=0.225

602 citations · 4.6k across the 33 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.HE2016★ 11 cited

First limits on the very-high energy gamma-ray afterglow emission of a fast radio burst: H.E.S.S. observations of FRB 150418

H. E. S. S. Collaboration, :, H. Abdalla +265

Aims: Following the detection of the fast radio burst FRB150418 by the SUPERB project at the Parkes radio telescope, we aim to search for very-high energy gamma-ray afterglow emiss…

astro-ph.HE2016★ 116 cited

H.E.S.S. observations of RX J1713.7-3946 with improved angular and spectral resolution; evidence for gamma-ray emission extending beyond the X-ray emitting shell

H. E. S. S. Collaboration, :, H. Abdalla +252

Supernova remnants exhibit shock fronts (shells) that can accelerate charged particles up to very high energies. In the past decade, measurements of a handful of shell-type superno…

astro-ph.HE2016★ 124 cited

Hitomi constraints on the 3.5 keV line in the Perseus galaxy cluster

Hitomi Collaboration, Felix A. Aharonian, Hiroki Akamatsu +215

High-resolution X-ray spectroscopy with Hitomi was expected to resolve the origin of the faint unidentified E=3.5 keV emission line reported in several low-resolution studies of va…

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