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R. Cassano

166 papers hereh-index 425.9k citations202 works total

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

author position
  • sole author3
  • first author17
  • middle author103
  • last author4

Across the 127 of 166 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO105
  • astro-ph22
  • astro-ph.GA20
  • astro-ph.HE15
  • astro-ph.IM4
same name
  • R. Cassano — 2 papers
  • R. Cassano — 1 paper
  • R. Cassano — 1 paper, h 0
  • R. Cassano — 1 paper, h 0

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
20032026
most citedThe LOFAR Two-metre Sky Survey - I. Survey Description and Preliminary Data Release

654 citations · 9.5k across the 164 of their papers we have counts for

collaborators
Showing 2007Show all

4 papers · 1 filter

astro-ph2007★ 62 cited

Revised statistics of radio halos and the re-acceleration model

R. Cassano, G. Brunetti, T. Venturi +4

Aims. The statistical properties of radio halos can be used to discriminate among the possible models for their origin. Therefore an unbiased and exhaustive investigation in this d…

astro-ph2007★ 158 cited

Cosmic rays and Radio Halos in galaxy clusters : new constraints from radio observations

G. Brunetti, T. Venturi, D. Dallacasa +4

Clusters of galaxies are sites of acceleration of charged particles and sources of non-thermal radiation. We report on new constraints on the population of cosmic rays in the Intra…

astro-ph2007

Hard X-rays from Galaxy Clusters and SIMBOL-X

G. Brunetti, R. Cassano, G. Setti

Non thermal emission from galaxy clusters demonstrates the existence of relativistic particles and magnetic fields in the Intra Cluster Medium (ICM). Present instruments do not all…

astro-ph2007★ 110 cited

New scaling relations in cluster radio halos and the re-acceleration model

R. Cassano, G. Brunetti, G. Setti +2

In this paper we derive new expected scaling relations for clusters with giant radio halos in the framework of the re-acceleration scenario in a simplified, but physically motivate…

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