Amiba and Galaxy Cluster Survey via Thermal Sunyaev-Zel Effects

Details Amiba and Galaxy Cluster Survey via Thermal Sunyaev-Zel Effects Amiba and Galaxy Cluster Survey via Thermal Sunyaev-Zel Effects

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cpa..conf...62c&link_type=abstract

PROCEEDINGS OF THE 2002 INTERNATIONAL SYMPOSIUM ON COSMOLOGY AND PARTICLE ASTROPHYSICS (CosPA 02). Held 31 May ?2 June 2002 in T

Astronomy and Astrophysics

Astrophysics

Scientific paper

Array for Microwave Background Anisotropy (AMiBA) is a 19-element, platform-mounted interferometry telescope operating at 90 GHz. With a 10' field of view and 2' angular resolution, the designed sensitivity of AMiBA for real-space imaging of galaxy clusters via the Sunyaev-Zel'dovich effect can achieve 150μ {K {K {√ {sec} } ; {√ {sec } }} . I present our preliminary tests for the quality of AMiBA cluster images via mosaic mock observations on the simulated sky produced by cosmological N-body/SPH simulations. I also discuss the issue of confusion caused by the synchrotron and dust emission from galaxies residing in clusters.

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