CaltechAUTHORS
Published January 27, 2020 | Version Submitted + Published
Journal Article Open

SZ contribution to characterize the shape of galaxy cluster haloes

Creators

  • 1. ROR icon INFN Sezione di Bologna
  • 2. ROR icon National Institute for Astrophysics
  • 3. ROR icon California Institute of Technology

Abstract

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.

Attached Files

Published - epjconf_mmuniverse2019_00009.pdf

Submitted - 1911.03247.pdf

Files

1911.03247.pdf

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Additional details

Identifiers

Eprint ID
101776
Resolver ID
CaltechAUTHORS:20200309-110008709

Related works

Describes
https://arxiv.org/abs/1911.03247 (URL)

Dates

Created
2020-03-09
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field