SZ contribution to characterize the shape of galaxy cluster haloes
We present the on-going activity to characterize the geometrical properties of the gas and dark matter haloes using multi-wavelength observations of galaxy clusters. The role of the SZ signal in describing the gas distribution is discussed for the pilot case of the CLASH object MACS J1206.2-0847.
Additional Information© 2020 The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/). Published online 27 January 2020.
Published - epjconf_mmuniverse2019_00009.pdf
Submitted - 1911.03247.pdf