https://doi.org/10.1051/epjconf/202022800009
SZ contribution to characterize the shape of galaxy cluster haloes
1
INAF, Osservatorio di Astrofisica e Scienza dello Spazio, via P. Gobetti 93/3, 40129 Bologna, Italy
2
INFN, Sezione di Bologna, viale Berti Pichat 6/2, I-40127 Bologna, Italy
3
INAF, Istituto di Radioastronomia – Italian ARC, via P. Gobetti 101, 40129, Bologna, Italy
4
California Institute of Technology, 200 E California Blvd., Pasadena, CA 91125
* e-mail: stefano.ettori@inaf.it
Published online: 27 January 2020
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.
© The Authors, published by EDP Sciences, 2020
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
