395 citations · 6.3k across the 105 of their papers we have counts for
8 papers · 2 filters
, a semi-analytic model for the thermodynamic properties in galaxy clusters: calibrations with mass and redshift, and implication for the hydrostatic bias
S. Ettori, L. Lovisari, D. Eckert
In the self-similar scenario for galaxy cluster formation and evolution, the thermodynamic properties of the X-ray emitting plasma can be predicted in their dependencies on the hal…
The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium
X. Zhang, A. Simionescu, F. Gastaldello +19
The footprint of LoTSS-DR2 covers 309 PSZ2 galaxy clusters, 83 of which host a radio halo and 26 host a radio relic(s). It provides us an excellent opportunity to statistically stu…
Joint HST, VLT/MUSE and XMM-Newton observations to constrain the mass distribution of the two strong lensing galaxy clusters: MACS J0242.5-2132 & MACS J0949.8+1708
Joseph F. V. Allingham, Mathilde Jauzac, David J. Lagattuta +6
We present the strong lensing analysis of two galaxy clusters: MACS J0242.5-2132 (MACS J0242, ) and MACS J0949.8+1708 (MACS J0949, ). Their total matter distribut…
CHEX-MATE: Morphological analysis of the sample
Maria Giulia Campitiello, Stefano Ettori, Lorenzo Lovisari +17
In this work, we performed an analysis of the X-ray morphology of the 118 CHEX-MATE (Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of…
Constraints on dark matter self-interaction from the internal density profiles of X-COP galaxy clusters
D. Eckert, S. Ettori, A. Robertson +4
TThe fundamental properties of the postulated dark matter (DM) affect the internal structure of gravitationally-bound structures. In the cold dark matter paradigm, DM particles int…
The gravitational field of X-COP galaxy clusters
D. Eckert, S. Ettori, E. Pointecouteau +2
The mass profiles of massive dark matter halos are highly sensitive to the nature of dark matter and potential modifications of the theory of gravity on large scales. The CDM pa…