activity
20022026
most citedThe effect of ram pressure on the star formation, mass distribution and morphology of galaxies

201 citations · 3k across the 63 of their papers we have counts for

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Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2021★ 3 cited

Gamma-ray detection toward the Coma cluster with Fermi-LAT: Implications for the cosmic ray content in the hadronic scenario

R. Adam, H. Goksu, S. Brown +2

The presence of relativistic electrons within the diffuse gas phase of galaxy clusters is now well established, but their detailed origin remains unclear. Cosmic ray protons are al…

astro-ph.HE2018★ 2 cited

SKA-Athena Synergy White Paper

R. Cassano, R. Fender, C. Ferrari +35

The Advanced Telescope for High Energy Astrophysics (Athena) is the X-ray observatory large mission selected by the European Space Agency (ESA), within its Cosmic Vision 2015-2025…

astro-ph.HE2016★ 156 cited

A large light-mass component of cosmic rays at 10^{17} - 10^{17.5} eV from radio observations

S. Buitink, A. Corstanje, H. Falcke +101

Cosmic rays are the highest energy particles found in nature. Measurements of the mass composition of cosmic rays between 10^{17} eV and 10^{18} eV are essential to understand whet…

astro-ph.HE2016★ 63 cited

A plethora of diffuse steep spectrum radio sources in Abell 2034 revealed by LOFAR

T. W. Shimwell, J. Luckin, M. Brüggen +28

With Low-Frequency Array (LOFAR) observations, we have discovered a diverse assembly of steep spectrum emission that is apparently associated with the intra cluster medium (ICM) of…

astro-ph.HE2016★ 185 cited

LOFAR, VLA, and Chandra observations of the Toothbrush galaxy cluster

R. J. van Weeren, G. Brunetti, M. Brüggen +39

We present deep LOFAR observations between 120-181 MHz of the "Toothbrush" (RX J0603.3+4214), a cluster that contains one of the brightest radio relic sources known. Our LOFAR obse…

astro-ph.HE2015★ 82 cited

Wide-Band, Low-Frequency Pulse Profiles of 100 Radio Pulsars with LOFAR

M. Pilia, J. W. T. Hessels, B. W. Stappers +84

LOFAR offers the unique capability of observing pulsars across the 10-240 MHz frequency range with a fractional bandwidth of roughly 50%. This spectral range is well-suited for stu…