| Issue |
EPJ Web Conf.
Volume 228, 2020
mm Universe @ NIKA2 - Observing the mm Universe with the NIKA2 Camera
|
|
|---|---|---|
| Article Number | 00009 | |
| Number of page(s) | 6 | |
| DOI | https://doi.org/10.1051/epjconf/202022800009 | |
| Published online | 27 January 2020 | |
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
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