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SZ contribution to characterize the shape of galaxy cluster haloes

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 نشر من قبل Stefano Ettori
 تاريخ النشر 2019
  مجال البحث فيزياء
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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. Preliminary images of the NIKA2 and ALMA exposures are presented.



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