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researcher

G. Brunetti

4 papers hereh-index 364 citations6 works total

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

author position
  • middle author3
  • last author1

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

fields
  • astro-ph.CO2
  • astro-ph1
  • hep-ex1
same name
  • G. Brunetti — 201 papers, h 55
  • G. Brunetti — 98 papers, h 17
  • G. Brunetti — 51 papers, h 23
  • G. Brunetti — 27 papers, h 19
  • G. Brunetti — 24 papers, h 8
  • G. Brunetti — 9 papers, h 3

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
20012026
most citedHard X-ray emission from the galaxy cluster A3667

45 citations · 47 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.CO2026

The Cosmic Ray Life Cycle in Galaxy Clusters

Francesco de Gasperin, Marcus Brüggen, Henrik Edler +3

Within the cosmic web, gravitational energy, linked to the formation and growth of the Universe's largest structures and the activity of active galactic nuclei (AGN), is converted…

hep-ex2026

Study of Supernova Neutrinos at ESSnuSB

ESSnuSB, :, J. Aguilar +97

In this paper, we have studied the sensitivity of the ESSnuSB far detector to supernova neutrinos. ESSnuSB is a proposed long-baseline neutrino experiment in Sweden, which will use…

astro-ph.CO2009★ 2 cited

Clusters and Large-Scale Structure: the Synchrotron Keys

L. Rudnick, P. Alexander, H. Andernach +25

For over four decades, synchrotron-radiating sources have played a series of pathfinding roles in the study of galaxy clusters and large scale structure. Such sources are uniquely…

astro-ph2001★ 45 cited

Hard X-ray emission from the galaxy cluster A3667

R. Fusco-Femiano, D. Dal Fiume, M. Orlandini +3

We report the results of a long BeppoSAX observation of Abell 3667, one of the most spectacular galaxy cluster in the southern sky. A clear detection of hard X-ray radiation up to…

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