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Communication Dans Un Congrès Année : 2020

NIKA: a mm camera for Sunyaev-Zel’dovich science in clusters of galaxies

R. Adam
P. Ade
  • Fonction : Auteur
H. Aussel
A. Beelen
M. Calvo
  • Fonction : Auteur
M. de Petris
  • Fonction : Auteur
S. Doyle
  • Fonction : Auteur
A. Gomez
  • Fonction : Auteur
G. Lagache
P. Mauskopf
  • Fonction : Auteur
L. Perotto
G. Pisano
  • Fonction : Auteur
F. Ruppin
  • Fonction : Auteur
C. Tucker
  • Fonction : Auteur

Résumé

Clusters of galaxies, the largest bound objects in the Universe, constitute a cosmological probe of choice, which is sensitive to both dark matter and dark energy. Within this framework, the Sunyaev-Zel’dovich (SZ) effect has opened a new window for the detection of clusters of galaxies and for the characterization of their physical properties such as mass, pressure and temperature. NIKA, a KID-based dual band camera installed at the IRAM 30-m telescope, was particularly well adapted in terms of frequency, angular resolution, field-of-view and sensitivity, for the mapping of the thermal and kinetic SZ effect in high-redshift clusters. In this paper, we present the NIKA cluster sample and a review of the main results obtained via the measurement of the SZ effect on those clusters: reconstruction of the cluster radial pressure profile, mass, temperature and velocity.

Dates et versions

hal-02448030 , version 1 (21-01-2020)

Identifiants

Citer

J.F. Macías-Pérez, R. Adam, P. Ade, P. André, A. Andrianasolo, et al.. NIKA: a mm camera for Sunyaev-Zel’dovich science in clusters of galaxies. mm Universe @ NIKA2, Jun 2019, Grenoble, France. pp.00016, ⟨10.1051/epjconf/202022800016⟩. ⟨hal-02448030⟩
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