output
20022026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing 2020 · astro-ph.HEShow all

22 papers · 2 filters

astro-ph.HE2020★ 55 cited

The impact of Solar wind variability on pulsar timing

C. Tiburzi, G. M. Shaifullah, C. G. Bassa +22

High-precision pulsar timing requires accurate corrections for dispersive delays of radio waves, parametrized by the dispersion measure (DM), particularly if these delays are varia…

astro-ph.HE2020★ 46 cited

Radio observations of the merging galaxy cluster system Abell 3391-Abell 3395

M. Brüggen, T. H. Reiprich, E. Bulbul +20

The pre-merging system of galaxy clusters Abell 3391-Abell 3395 located at a mean redshift of 0.053 has been observed at 1 GHz in an ASKAP/EMU Early Science observation as well as…

astro-ph.HE2020★ 45 cited

Dispersion measure variability for 36 millisecond pulsars at 150MHz with LOFAR

J. Y. Donner, J. P. W. Verbiest, C. Tiburzi +19

Radio pulses from pulsars are affected by plasma dispersion, which results in a frequency-dependent propagation delay. Variations in the magnitude of this effect lead to an additio…

astro-ph.HE2020★ 23 cited

Diffuse Radio Emission from Galaxy Clusters in the LOFAR Two-metre Sky Survey Deep Fields

E. Osinga, R. J. van Weeren, J. Boxelaar +15

Low-frequency radio observations are revealing an increasing number of diffuse synchrotron sources from galaxy clusters, dominantly in the form of radio halos or radio relics. The…

astro-ph.HE2020★ 13 cited

LOFAR Detection of a Low-Power Radio Halo in the Galaxy Cluster Abell 990

N. D. Hoang, T. W. Shimwell, E. Osinga +10

Radio halos are extended (), steep-spectrum sources found in the central region of dynamically disturbed clusters of galaxies. Only a handful of radio halos have bee…

astro-ph.HE2020★ 9 cited

ClG 0217+70: A massive merging galaxy cluster with a large radio halo and relics

X. Zhang, A. Simionescu, J. S. Kaastra +7

We present an analysis of archival Chandra data of the merging galaxy cluster ClG 0217+70. The Fe XXV He X-ray emission line is clearly visible in the 25 ks observation, allowin…