Testing Cosmological SZE-X-ray-Multi-Wavelength Galaxy Cluster Surveys

Details Testing Cosmological SZE-X-ray-Multi-Wavelength Galaxy Cluster Surveys Testing Cosmological SZE-X-ray-Multi-Wavelength Galaxy Cluster Surveys

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008xmm..prop..132b&link_type=abstract

XMM-Newton Proposal ID #06048703

Physics

Cosmology, Extragalactic Deep Fields And Area Surveys, Survey_Mosaic_1, Survey_Mosaic_2, Survey_Mosaic_3

Scientific paper

Sunyaev-Zeldovich Effect (SZE) surveys have finally and successfully opened a new window to study the cosmic large-scale structure in a more promising way than previous methods. We have performed a coordinated SZE, X-ray, and optical/MIR survey to best understand the potential of this new survey technique and obtained the first exciting multi-wavelength detections. Here we propose to extent the current small test area applying the new XMM-Newton mosaic mode, which allows us to adapt our survey optimally to the depth of the SZE surveys allowing for about 100 cluster detections with XMM.

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