activity
20182020
most citedThe beautiful mess in Abell 2255

86 citations · 100 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph.GA202086 cited

The beautiful mess in Abell 2255

A. Botteon, G. Brunetti, R. J. van Weeren +18

We present LOFAR observations of one of the most spectacular objects in the radio sky: Abell 2255. This is a nearby () merging galaxy cluster hosting one of the first r…

astro-ph.IM20191 cited

Realising the LOFAR Two-Metre Sky Survey -- using the supercomputer JUWELS at the Forschungszentrum Jülich

A. Drabent, M. Hoeft, A. P. Mechev +10

The new generation of high-resolution broad-band radio telescopes, like the Low Frequency Array (LOFAR), produces, depending on the level of compression, between 1 to 10 TB of data…

astro-ph.HE2019

New mysteries and challenges from the Toothbrush relic: wideband observations from 550 MHz to 8 GHz

K. Rajpurohit, M. Hoeft, F. Vazza +10

Radio relics are diffuse extended synchrotron sources that originate from shock fronts induced by galaxy cluster mergers. The actual particle acceleration mechanism at the shock fr…

astro-ph.SR201913 cited

The first detection of a low-frequency turnover in nonthermal emission from the jet of a young star

Anton Feeney-Johansson, Simon J. D. Purser, Tom P. Ray +4

Radio emission in jets from young stellar objects (YSOs) in the form of nonthermal emission has been seen toward several YSOs. Thought to be synchrotron emission from strong shocks…

astro-ph.CO2018

Ultra-steep spectrum emission in the merging galaxy cluster Abell 1914

S. Mandal, H. T. Intema, T. W. Shimwell +14

A number of radio observations have revealed the presence of large synchrotron-emitting sources associated with the intra-cluster medium. There is strong observational evidence tha…

astro-ph.CO2018

A LOFAR study of non-merging massive galaxy clusters

Federica Savini, Annalisa Bonafede, Marcus Brueggen +15

Centrally located diffuse radio emission has been observed in both merging and non-merging galaxy clusters. Depending on their morphology and size, we distinguish between giant rad…