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Alison M. W. Mitchell

3 papers here

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

author position
  • first author1
  • last author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3

identity via Semantic Scholar / OpenAlex

most citedTeV Emission from PSR B1055-52 with HESS: Evidence for a Pulsar Halo

2 citations · 2 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025

Joint eROSITA and H.E.S.S. analysis of MSH 15-52 using Gammapy

Katharina Egg, Alison M. W. Mitchell

Pulsar wind nebulae (PWNe) are prominent sources in the very-high energy (VHE) gamma-ray sky, constituting the most numerous identified source class in the H.E.S.S. Galactic Plane…

astro-ph.HE2025

Analysis of the Supernova Remnant IC 443 using H.E.S.S. Data

Alison M. W. Mitchell, Lukas Grosspietsch, Tina Wach

IC 443 is a well-known supernova remnant that stands out due to its interaction with a dense molecular cloud, creating a complex environment where shocks can efficiently accelerate…

astro-ph.HE2025★ 2 cited

TeV Emission from PSR B1055-52 with HESS: Evidence for a Pulsar Halo

Tina Wach, Alison M. W. Mitchell

Pulsar halos are a recently identified class of TeV γ-ray sources, offering valuable insights into the evolution of pulsar systems at the highest energies. However, only a handfu…

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