395 citations · 4.1k across the 114 of their papers we have counts for
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The unusually weak and exceptionally steep radio relic in Abell 2108
Gerrit Schellenberger, Simona Giacintucci, Lorenzo Lovisari +9
Mergers between galaxy clusters often drive shocks into the intra cluster medium (ICM), the effects of which are sometimes visible via temperature and density jumps in the X-ray, a…
On the dynamical and morphological state of the CHEX-MATE clusters
Maria Giulia Campitiello, Stefano Ettori, Lorenzo Lovisari +1
The CHEX-MATE sample was built to provide an overview of the statistical properties of the underlying cluster population and to set the stage for future X-ray missions. In this wor…
The thermalisation of massive galaxy clusters
Mauro Sereno, Lorenzo Lovisari, Weiguang Cui +1
In the hierarchical scenario of structure formation, galaxy clusters are the ultimate virialised products in mass and time. Hot baryons in the intracluster medium (ICM) and cold ba…
Scaling Properties of Galaxy Groups
Lorenzo Lovisari, Stefano Ettori, Massimo Gaspari +1
Galaxy groups and poor clusters are more common than rich clusters, and host the largest fraction of matter content in the Universe. Hence, their studies are key to understand the…
Chandra Observations of the Planck ESZ Sample: A Re-Examination of Masses and Mass Proxies
Felipe Andrade-Santos, Gabriel W. Pratt, Jean-Baptiste Melin +14
Using Chandra observations, we derive the proxy and associated total mass measurement, , for 147 clusters with from the Planck Early Su…
Cosmological implications of the anisotropy of ten galaxy cluster scaling relations
K. Migkas, F. Pacaud, G. Schellenberger +5
The hypothesis that the late Universe is isotropic and homogeneous is adopted by most cosmological studies. The expansion rate is thought to be spatially constant, while bulk…
The intra-cluster magnetic field in the double relic galaxy cluster Abell 2345
C. Stuardi, A. Bonafede, L. Lovisari +5
Magnetic fields are ubiquitous in galaxy clusters, yet their radial profile, power spectrum, and connection to host cluster properties are poorly known. Merging galaxy clusters hos…