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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.

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Bibliografiset tiedot
Päätekijät: Ettori Stefano, Sereno Mauro, Burkutean Sandra, Sayers Jack
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: EDP Sciences 2020-01-01
Sarja:EPJ Web of Conferences
Linkit:https://www.epj-conferences.org/articles/epjconf/pdf/2020/04/epjconf_mmuniverse2019_00009.pdf
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