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researcher

D. Hoffmann

26 papers hereh-index 9938 citations34 works total

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

author position
  • middle author10
  • last author1

Across the 11 of 26 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE19
  • astro-ph.IM6
  • physics.ins-det1
same name
  • D. Hoffmann — 142 papers
  • D. Hoffmann — 86 papers, h 20
  • D. Hoffmann — 40 papers, h 0
  • D. Hoffmann — 22 papers, h 7
  • D. Hoffmann — 20 papers, h 21
  • D. Hoffmann — 19 papers, h 42

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
20102026
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 1.2k across the 25 of their papers we have counts for

collaborators
Showing 2023 · astro-ph.HEShow all

3 papers · 2 filters

astro-ph.HE2023★ 9 cited

Prospects for γ-ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array

The Cherenkov Telescope Array Consortium, :, K. Abe +564

Galaxy clusters are expected to be dark matter (DM) reservoirs and storage rooms for the cosmic-ray protons (CRp) that accumulate along the cluster's formation history. Accordingly…

astro-ph.HE2023★ 50 cited

Observations of the Crab Nebula and Pulsar with the Large-Sized Telescope Prototype of the Cherenkov Telescope Array

CTA-LST Project, :, H. Abe +289

CTA (Cherenkov Telescope Array) is the next generation ground-based observatory for gamma-ray astronomy at very-high energies. The Large-Sized Telescope prototype (LST-1) is locate…

astro-ph.HE2023★ 22 cited

Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

The Cherenkov Telescope Array Consortium, F. Acero, A. Acharyya +356

The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3~PeV. Sources which are capable of accelerating hadrons to such energies are called hadr…

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