172 citations · 997 across the 14 of their papers we have counts for
16 papers
Turbulence and Particle Acceleration in Giant Radio Haloes: the Origin of Seed Electrons
Anders Pinzke, S. Peng Oh, Christoph Pfrommer
About 1/3 of X-ray-luminous clusters show smooth, Mpc-scale radio emission, known as giant radio haloes. One promising model for radio haloes is Fermi-II acceleration of seed relat…
Deep observation of the NGC 1275 region with MAGIC: search of diffuse gamma-ray emission from cosmic rays in the Perseus cluster
MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +154
Clusters of galaxies are expected to be reservoirs of cosmic rays (CRs) that should produce diffuse gamma-ray emission due to their hadronic interactions with the intra-cluster med…
Constraints on the cosmic ray cluster physics from a very deep observation of the Perseus cluster with MAGIC
Pierre Colin, Fabio Zandanel, Monica Vazquez Acosta +3
Galaxy clusters are the largest and most massive gravitationally bound structures known in the Universe. Cosmic-Ray (CR) hadrons accelerated at structure formation shocks and injec…
Turbulence and Particle Acceleration in Giant Radio Halos: the Origin of Seed Electrons
Anders Pinzke, S. Peng Oh, Christoph Pfrommer
About 1/3 of X-ray-luminous clusters show smooth, unpolarized radio emission on ~Mpc scales, known as giant radio halos. One promising model for radio halos is Fermi-II acceleratio…
MAGIC Gamma-ray Observations of the Perseus Galaxy Cluster
Fabio Zandanel, Pierre Colin, Saverio Lombardi +6
In order to detect the gamma-ray emission from cosmic ray (CR) interactions with the intra-cluster medium, the ground-based imaging Cherenkov telescope MAGIC conducted the deepest-…
Giant radio relics in galaxy clusters: reacceleration of fossil relativistic electrons?
Anders Pinzke, S. Peng Oh, Christoph Pfrommer
Many bright radio relics in the outskirts of galaxy clusters have low inferred Mach numbers, defying expectations from shock acceleration theory and heliospheric observations that…